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Statistics

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# What Is Statistics?

Your company has created a new drug that may cure arthritis. How would you conduct a test to confirm the drug's effectiveness?

The latest sales data have just come in, and your boss wants you to prepare a report for management on places where the company could improve its business. What should you look for? What should you not look for?

You and a friend are at a baseball game, and out of the blue he offers you a bet that neither team will hit a home run in that game. Should you take the bet?

You want to conduct a poll on whether your school should use its funding to build a new athletic complex or a new library. How many people do you have to poll? How do you ensure that your poll is free of bias? How do you interpret your results?

A widget maker in your factory that normally breaks 4 widgets for every 100 it produces has recently started breaking 5 widgets for every 100. When is it time to buy a new widget maker? (And just what is a widget, anyway?)

These are some of the many real-world examples that require the use of statistics.

## General Definition

Statistics, in short, is the study of data. It includes descriptive statistics (the study of methods and tools for collecting data, and mathematical models to describe and interpret data) and inferential statistics (the systems and techniques for making probability-based decisions and accurate predictions based on incomplete (sample) data).

# Subjects in Modern Statistics

## Modern Statistics

A remarkable amount of today's modern statistics comes from the original work of R.A. Fisher in the early 20th Century. Although there are a dizzying number of minor disciplines in the field, there are some basic, fundamental studies. The beginning student of statistics will be more interested in one topic or another depending on his or her outside interest. The following is a list of some of the primary branches of statistics.

### Probability Theory and Mathematical Statistics

Those of us who are purists and philosophers may be interested in the union between pure mathematics and the messy realities of the world. A rigorous study of probability—especially the probability distributions and the distribution of errors—can provide an understanding of where all these statistical procedures and equations come from. Although this sort of rigor is likely to get in the way of a psychologist (for example) learning and using statistics effectively, it is important if one wants to do serious (i.e. graduate-level) work in the field.

That being said, there is good reason for all students to have a fundamental understanding of where all these "statistical techniques and equations" are coming from! We're always more adept at using a tool if we can understand why we're using that tool. The challenge is getting these important ideas to the non-mathematician without the student's eyes glazing over. One can take this argument a step further to claim that a vast number of students will never actually use a t-test—he or she will never plug those numbers into a calculator and churn through some esoteric equations—but by having a fundamental understanding of such a test, he or she will be able to understand (and question) the results of someone else's findings.

### Design of Experiments

One of the most neglected aspects of statistics—and maybe the single greatest reason that Statisticians drink—is Experimental Design. So often a scientist will bring the results of an important experiment to a statistician and ask for help analyzing results only to find that a flaw in the experimental design rendered the results useless. So often we statisticians have researchers come to us hoping that we will somehow magically "rescue" their experiments.

A friend provided me with a classic example of this. In his psychology class he was required to conduct an experiment and summarize its results. He decided to study whether music had an impact on problem solving. He had a large number of subjects (myself included) solve a puzzle first in silence, then while listening to classical music and finally listening to rock and roll, and finally in silence. He measured how long it would take to complete each of the tasks and then summarized the results.

What my friend failed to consider was that the results were highly impacted by a learning effect he hadn't considered. The first puzzle always took longer because the subjects were first learning how to work the puzzle. By the third try (when subjected to rock and roll) the subjects were much more adept at solving the puzzle, thus the results of the experiment would seem to suggest that people were much better at solving problems while listening to rock and roll!

The simple act of randomizing the order of the tests would have isolated the "learning effect" and in fact, a well-designed experiment would have allowed him to measure both the effects of each type of music and the effect of learning. Instead, his results were meaningless. A careful experimental design can help preserve the results of an experiment, and in fact some designs can save huge amounts of time and money, maximize the results of an experiment, and sometimes yield additional information the researcher had never even considered!

### Sampling

Similar to the Design of Experiments, the study of sampling allows us to find a most effective statistical design that will optimize the amount of information we can collect while minimizing the level of effort. Sampling is very different from experimental design however. In a laboratory we can design an experiment and control it from start to finish. But often we want to study something outside of the laboratory, over which we have much less control.

If we wanted to measure the population of some harmful beetle and its effect on trees, we would be forced to travel into some forest land and make observations, for example: measuring the population of the beetles in different locations, noting which trees they were infesting, measuring the health and size of these trees, etc.

Sampling design gets involved in questions like "How many measurements do I have to take?" or "How do I select the locations from which I take my measurements?" Without planning for these issues, researchers might spend a lot of time and money only to discover that they really have to sample ten times as many points to get meaningful results or that some of their sample points were in some landscape (like a marsh) where the beetles thrived more or the trees grew better.

### Modern Regression

Regression models relate variables to each other in a linear fashion. For example, if you recorded the heights and weights of several people and plotted them against each other, you would find that as height increases, weight tends to increase too. You would probably also see that a straight line through the data is about as good a way of approximating the relationship as you will be able to find, though there will be some variability about the line. Such linear models are possibly the most important tool available to statisticians. They have a long history and many of the more detailed theoretical aspects were discovered in the 1970s. The usual method for fitting such models is by "least squares" estimation, though other methods are available and are often more appropriate, especially when the data are not normally distributed.

What happens, though, if the relationship is not a straight line? How can a curve be fit to the data? There are many answers to this question. One simple solution is to fit a quadratic relationship, but in practice such a curve is often not flexible enough. Also, what if you have many variables and relationships between them are dissimilar and complicated?

Modern regression methods aim at addressing these problems. Methods such as generalized additive models, projection pursuit regression, neural networks and boosting allow for very general relationships between explanatory variables and response variables, and modern computing power makes these methods a practical option for many applications

### Classification

Some things are different from others. How? That is, how are objects classified into their respective groups? Consider a bank that is hoping to lend money to customers. Some customers who borrow money will be unable or unwilling to pay it back, though most will pay it back as regular repayments. How is the bank to classify customers into these two groups when deciding which ones to lend money to?

The answer to this question no doubt is influenced by many things, including a customer's income, credit history, assets, already existing debt, age and profession. There may be other influential, measurable characteristics that can be used to predict what kind of customer a particular individual is. How should the bank decide which characteristics are important, and how should it combine this information into a rule that tells it whether or not to lend the money?

This is an example of a classification problem, and statistical classification is a large field containing methods such as linear discriminant analysis, classification trees, neural networks and other methods.

### Time Series

Many types of research look at data that are gathered over time, where an observation taken today may have some correlation with the observation taken tomorrow. Two prominent examples of this are the fields of finance (the stock market) and atmospheric science.

We've all seen those line graphs of stock prices as they meander up and down over time. Investors are interested in predicting which stocks are likely to keep climbing (i.e. when to buy) and when a stock in their portfolio is falling. It is easy to be misled by a sudden jolt of good news or a simple "market correction" into inferring—incorrectly—that one or the other is taking place!

In meteorology scientists are concerned with the venerable science of predicting the weather. Whether trying to predict if tomorrow will be sunny or determining whether we are experiencing true climate changes (i.e. global warming) it is important to analyze weather data over time.

### Survival Analysis

Suppose that a pharmaceutical company is studying a new drug which it is hoped will cause people to live longer (whether by curing them of cancer, reducing their blood pressure or cholesterol and thereby their risk of heart disease, or by some other mechanism). The company will recruit patients into a clinical trial, give some patients the drug and others a placebo, and follow them until they have amassed enough data to answer the question of whether, and by how long, the new drug extends life expectancy.

Such data present problems for analysis. Some patients will have died earlier than others, and often some patients will not have died before the clinical trial completes. Clearly, patients who live longer contribute informative data about the ability (or not) of the drug to extend life expectancy. So how should such data be analysed?

Survival analysis provides answers to this question and gives statisticians the tools necessary to make full use of the available data to correctly interpret the treatment effect.

### Categorical Analysis

In laboratories we can measure the weight of fruit that a plant bears, or the temperature of a chemical reaction. These data points are easily measured with a yardstick or a thermometer, but what about the color of a person's eyes or her attitudes regarding the taste of broccoli? Psychologists can't measure someone's anger with a measuring stick, but they can ask their patients if they feel "very angry" or "a little angry" or "indifferent". Entirely different methodologies must be used in statistical analysis from these sorts of experiments. Categorical Analysis is used in a myriad of places, from political polls to analysis of census data to genetics and medicine.

### Clinical Trials

In the United States, the FDA requires that pharmaceutical companies undergo excruciatingly rigorous procedures called Clinical Trials and statistical analyses to assure public safety before allowing the sale of use of new drugs. In fact, the pharmaceutical industry employs more statisticians than any other business!

# Different Types of Data

Data are assignments of values onto observations of events and objects. They can be classified by their coding properties and the characteristics of their domains and their ranges.

## Identifying data type

When a given data set is numerical in nature, it is necessary to carefully distinguish the actual nature of the variable being quantified. Statistical tests are generally specific for the kind of data being handled.

### Data on a nominal (or categorical) scale

Identifying the true nature of numerals applied to attributes that are not "measures" is usually straightforward and apparent. Examples in everyday use include road, car, house, book and telephone numbers. A simple test would be to ask if re-assigning the numbers among the set would alter the nature of the collection. If the plates on a car are changed, for example, it still remains the same car.

### Data on an ordinal (rank) scale

The use of numerals to assign arbitrary points along an otherwise unmeasurable continuum is often carried out in science.

An example would be grading the hair color of a collection of people, by making white = 0 and black = 5, say. Then points 2, 3 and 4 would involve subjective judgement concerning red, yellow and brown hair types, as well as variation due to random scoring of intermediates because of different environmental conditions. Notice that another ordinal scale, the alphabet, could equally well be used, assigning white = A and black = E. All that is necessary is to agree the rank order of the letters in the alphabet ABCDE.

Numerical ranked data can be distinguished from measurement data by noting that differences such as (3) - (2) only have meaning in the sense that (3) > (2). In the hair color example, it would be meaningless to have a value for the difference between blonde and chestnut, though one might agree that chestnut is closer to black and blonde is closer to white. Even if values were possible, for example by using some kind of color comparator, the data may still not be measurement data. For variates to be measurements, their differences would have values which in the simplest cases would all be the same - and at least proportional to each other.

To test if the differences really are meaningful and the corresponding variates are true measurements, imagine forming ratios between the differences. Ranked variates would not form sensible ratios for, say, (3)-(2)/(4)-(3).

### Measurement data

Numerical measurements exist in two forms, meristic and continuous, and may present themselves in three kinds of scale: interval, ratio and circular.

Meristic or discrete variables are generally counts and can take on only discrete values. Normally they are represented by natural numbers. The number of plants found in a botanist's quadrat would be an example. (Note that if the edge of the quadrat falls partially over one or more plants, the investigator may choose to include these as halves, but the data will still be meristic as doubling the total will remove any fraction).

Continuous variables are those whose measurement precision is limited only by the investigator and his equipment. The length of a leaf measured by a botanist with a ruler will be less precise than the same measurement taken by micrometer. (Notionally, at least, the leaf could be measured even more precisely using a microscope with a graticule.)

Interval Scale Variables measured on an interval scale have values in which differences are uniform and meaningful but ratios will not be so. An oft quoted example is that of the Celsius scale of temperature. A difference between 5° and 10° is equivalent to a difference between 10° and 15°, but the ratio between 15° and 5° does not imply that the former is three times as warm as the latter.

Ratio Scale Variables on a ratio scale have a meaningful zero point. In keeping with the above example one might cite the Kelvin temperature scale. Because there is an absolute zero, it is true to say that 400°K is twice as warm as 200°K, though one should do so with tongue in cheek. A better day-to-day example would be to say that a 180 kg Sumo wrestler is three times heavier than his 60 kg wife.

Circular Scale When one measures annual dates, clock times and a few other forms of data, a circular scale is in use. It can happen that neither differences nor ratios of such variables are sensible derivatives, and special methods have to be employed for such data.

# Primary and Secondary Data

## Primary and Secondary Data

Data can be classified as either primary or secondary.

### Primary Data

Primary data means original data that have been collected specially for the purpose in mind.

Research where one gathers this kind of data is referred to as field research .

For example: a questionnaire.

### Secondary Data

Secondary data are data that have been collected for another purpose and where we will use Statistical Method with the Primary Data. It means that after performing statistical operations on Primary Data the results become known as Secondary Data.

Research where one gathers this kind of data is referred to as desk research .

For example: data from a book.

# Quantitative and Qualitative Data

Quantitative and qualitative data are two types of data.

Qualitative data Qualitative - or categorical measurement expressed not in terms of numbers, but rather by means of a natural language description. In statistics it is often used interchangeably with "categorical" data.

  For example: favourite colour = "blue"
height = "tall"


Although we may have categories, the categories may have a structure to them. When there is not a natural ordering of the categories, we call these nominal categories. Examples might be gender, race, religion, or sport.

When the categories may be ordered, these are called ordinal variables. Categorical variables that judge size (small, medium, large, etc.) are ordinal variables. Attitudes (strongly disagree, disagree, neutral, agree, strongly agree) are also ordinal variables, however we may not know which value is the best or worst of these issues. Note that the distance between these categories is not something we can measure.

## Quantitative data

Quantitative -- or numerical measurement expressed not by means of a natural language description, but rather in terms of numbers. However, not all numbers are continuous and measurable -- for example social security number -- even though it is a number it is not something that one can add or subtract.

  For example: favourite colour = "450 nm"
height = "1.8 m"


Quantitative data always are associated with a scale measure.

Probably the most common scale type is the ratio-scale. Observations of this type are on a scale that has a meaningful zero value but also have an equidistant measure (i.e., the difference between 10 and 20 is the same as the difference between 100 and 110). For example a 10 year-old girl is twice as old as a 5 year-old girl. Since you can measure zero years, time is a ratio-scale variable. Money is another common ratio-scale quantitative measure. Observations that you count are usually ratio-scale (e.g., number of widgets).

A more general quantitative measure is the interval scale. Interval scales also have a equidistant measure. However, the doubling principle breaks down in this scale. A temperature of 50 degrees Celsius is not "half as hot" as a temperature of 100, but a difference of 10 degrees indicates the same difference in temperature anywhere along the scale. The Kelvin temperature scale, however, constitutes a ratio scale because on the Kelvin scale zero indicates absolute zero in temperature, the complete absence of heat. So one can say, for example, that 200 degrees Kelvin is twice as hot as 100 degrees Kelvin.

# Methods of Data Collection

Four Methods

Textular Method
Tabular Method
provides a more precise, systematic and orderly presentation of data in rows or columns.
Semi-tabular Method
uses both textual and tabular methods.
Graphical Method
the utilization of graphs is most effective method of presenting statistical results or findings.

# Experiments

## Experiments

It's true that scientists utilize two methods to gather information about the world: correlations (a.k.a. observational research) and experiments.

Experiments, no matter the scientific field, all have two distinct variables. Firstly, an independent variable (IV) is manipulated by an experimenter to exist in at least two levels (usually "none" and "some"). Then the experimenter measures the second variable, the dependent variable (DV).

A simple example---

Suppose the experimental hypothesis that concerns the scientist is that reading a Wiki will enhance knowledge. Notice that the hypothesis is really an attempt to state a causal relationship like, "if you read a Wiki, then you will have enhanced knowledge." The antecedent condition (reading a Wiki) causes the consequent condition (enhanced knowledge). Antecedent conditions are always IVs and consequent conditions are always DVs in experiments. So the experimenter would produce two levels of Wiki reading (none and some, for example) and record knowledge. If the subjects who got no Wiki exposure had less knowledge than those who were exposed to Wikis, it follows that the difference is caused by the IV.

So, the reason scientists utilize experiments is that it is the only way to determine causal relationships between variables. Experiments tend to be artificial because they try to make both groups identical with the single exception of the levels of the independent variable.

# Sample Surveys

Sample surveys involve the selection and study of a sample of items from a population. A sample is just a set of members chosen from a population, but not the whole population. A survey of a whole population is called a census.

Examples of sample surveys:

• Phoning the fifth person on every page of the local phonebook and asking them how long they have lived in the area. (Systematic Sample)
• Dropping a quad. in five different places on a field and counting the number of wild flowers inside the quad. (Cluster Sample)
• Selecting sub-populations in proportion to their incidence in the overall population. For instance, a researcher may have reason to select a sample consisting 30% females and 70% males in a population with those same gender proportions. (Stratified Sample)
• Selecting several cities in a country, several neighbourhoods in those cities and several streets in those neighbourhoods to recruit participants for a survey (Multi-stage sample)

The term random sample is used for a sample in which every item in the population is equally likely to be selected.

# Observational Studies

The most primitive method of understanding the laws of nature utilizes observational studies. Basically, a researcher goes out into the world and looks for variables that are associated with one another. Notice that, unlike experiments, observational research had no Independent Variables --- nothing is manipulated by the experimenter. Rather, observations (also called correlations, after the statistical techniques used to analyze the data) have the equivalent of two Dependent Variables.

Some of the foundations of modern scientific thought are based on observational research. Charles Darwin, for example, based his explanation of evolution entirely on observations he made. Case studies, where individuals are observed and questioned to determine possible causes of problems, are a form of observational research that continues to be popular today. In fact, every time you see a physician he or she is performing observational science.

There is a problem in observational science though --- it cannot ever identify causal relationships because even though two variables are related both might be caused by a third, unseen, variable. Since the underlying laws of nature are assumed to be causal laws, observational findings are generally regarded as less compelling than experimental findings.**

Observational data are more prevalent in describing large systems like in Astronomy, Economics, or Sociology, while subjects like Physics and Psychology can be more easily subject to experiments, when they don't involve large systems, which can't be artificially constructed as easily.

# Data Analysis

Data analysis is one of the more important stages in our research. Without performing exploratory analyses of our data, we set ourselves up for mistakes and loss of time.

Generally speaking, our goal here is to be able to "visualize" the data and get a sense of their values. We plot histograms and compute summary statistics to observe the trends and the distribution of our data.

# Data Cleaning

'Cleaning' refers to the process of removing invalid data points from a dataset.

Many statistical analyses try to find a pattern in a data series, based on a hypothesis or assumption about the nature of the data. 'Cleaning' is the process of removing those data points which are either (a) Obviously disconnected with the effect or assumption which we are trying to isolate, due to some other factor which applies only to those particular data points. (b) Obviously erroneous, i.e. some external error is reflected in that particular data point, either due to a mistake during data collection, reporting etc.

In the process we ignore these particular data points, and conduct our analysis on the remaining data.

'Cleaning' frequently involves human judgement to decide which points are valid and which are not, and there is a chance of valid data points caused by some effect not sufficiently accounted for in the hypothesis/assumption behind the analytical method applied.

The points to be cleaned are generally extreme outliers. 'Outliers' are those points which stand out for not following a pattern which is generally visible in the data. One way of detecting outliers is to plot the data points (if possible) and visually inspect the resultant plot for points which lie far outside the general distribution. Another way is to run the analysis on the entire dataset, and then eliminating those points which do not meet mathematical 'control limits' for variability from a trend, and then repeating the analysis on the remaining data.

Cleaning may also be done judgementally, for example in a sales forecast by ignoring historical data from an area/unit which has a tendency to misreport sales figures. To take another example, in a double blind medical test a doctor may disregard the results of a volunteer whom the doctor happens to know in a non-professional context.

'Cleaning' may also sometimes be used to refer to various other judgemental/mathematical methods of validating data and removing suspect data.

The importance of having clean and reliable data in any statistical analysis cannot be stressed enough. Often, in real-world applications the analyst may get mesmerised by the complexity or beauty of the method being applied, while the data itself may be unreliable and lead to results which suggest courses of action without a sound basis. A good statistician/researcher (personal opinion) spends 90% of his/her time on collecting and cleaning data, and developing hypothesis which cover as many external explainable factors as possible, and only 10% on the actual mathematical manipulation of the data and deriving results.

# Summary Statistics

## Summary Statistics

The most simple example of statistics "in practice" is in the generation of summary statistics. Let us consider the example where we are interested in the weight of eighth graders in a school. (Maybe we're looking at the growing epidemic of child obesity in America!) Our school has 200 eighth graders, so we gather all their weights. What we have are 200 positive real numbers.

If an administrator asked you what the weight was of this eighth grade class, you wouldn't grab your list and start reading off all the individual weights; it's just too much information. That same administrator wouldn't learn anything except that she shouldn't ask you any questions in the future! What you want to do is to distill the information — these 200 numbers — into something concise.

What might we express about these 200 numbers that would be of interest? The most obvious thing to do is to calculate the average or mean value so we know how much the "typical eighth grader" in the school weighs. It would also be useful to express how much this number varies; after all, eighth graders come in a wide variety of shapes and sizes! In reality, we can probably reduce this set of 200 weights into at most four or five numbers that give us a firm comprehension of the data set.

# Range of the Data

The range of a sample (set of data) is simply the maximum possible difference in the data, i.e. the difference between the maximum and the minimum values. A more exact term for it is "range width" and is usually denoted by the letter R or w. The two individual values (the max. and min.) are called the "range limits". Often these terms are confused and students should be careful to use the correct terminology.

For example, in a sample with values 2 3 5 7 8 11 12, the range is 10 and the range limits are 2 and 12.

The range is the simplest and most easily understood measure of the dispersion (spread) of a set of data, and though it is very widely used in everyday life, it is too rough for serious statistical work. It is not a "robust" measure, because clearly the chance of finding the maximum and minimum values in a population depends greatly on the size of the sample we choose to take from it and so its value is likely to vary widely from one sample to another. Furthermore, it is not a satisfactory descriptor of the data because it depends on only two items in the sample and overlooks all the rest. A far better measure of dispersion is the standard deviation (s), which takes into account all the data. It is not only more robust and "efficient" than the range, but is also amenable to far greater statistical manipulation. Nevertheless the range is still much used in simple descriptions of data and also in quality control charts.

The mean range of a set of data is however a quite efficient measure (statistic) and can be used as an easy way to calculate s. What we do in such cases is to subdivide the data into groups of a few members, calculate their average range, $\bar{R}$ and divide it by a factor (from tables), which depends on n. In chemical laboratories for example, it is very common to analyse samples in duplicate, and so they have a large source of ready data to calculate s.

$s= \frac {\bar{R}}k$

(The factor k to use is given under standard deviation.)

For example: If we have a sample of size 40, we can divide it into 10 sub-samples of n=4 each. If we then find their mean range to be, say, 3.1, the standard deviation of the parent sample of 40 items is appoximately 3.1/2.059 = 1.506.

With simple electronic calculators now available, which can calculate s directly at the touch of a key, there is no longer much need for such expedients, though students of statistics should be familiar with them.

# Quartiles

## Quartiles

The quartiles of a data set are formed by the two boundaries on either side of the median, which divide the set into four equal sections. The lowest 25% of the data being found below the first quartile value, also called the lower quartile (Q1). The median, or second quartile divides the set into two equal sections. The lowest 75% of the data set should be found below the third quartile, also called the upper quartile (Q3). These three numbers are measures of the dispersion of the data, while the mean, median and mode are measures of central tendency.

### Examples

Given the set {1, 3, 5, 8, 9, 12, 24, 25, 28, 30, 41, 50} we would find the first and third quartiles as follows:

There are 12 elements in the set, so 12/4 gives us three elements in each quarter of the set.

So the first or lowest quartile is: 5, the second quartile is the median 12, and the third or upper quartile is 28.

However some people when faced with a set with an even number of elements (values) still want the true median (or middle value), with an equal number of data values on each side of the median (rather than 12 which has 5 values less than and 6 values greater than. This value is then the average of 12 and 24 resulting in 18 as the true median (which is closer to the mean of 19 2/3. The same process is then applied to the lower and upper quartiles, giving 6.5, 18, and 29. This is only an issue if the data contains an even number of elements with an even number of equally divided sections, or an odd number of elements with an odd number of equally divided sections.

### Inter-Quartile Range

The inter quartile range is a statistic which provides information about the spread of a data set, and is calculated by subtracting the first quartile from the third quartile), giving the range of the middle half of the data set, trimming off the lowest and highest quarters. Since the IQR is not affected at all by outliers in the data, it is a more robust measure of dispersion than the range

IQR = Q3 - Q1

Another useful quantile is the quintiles which subdivide the data into five equal sections. The advantage of quintiles is that there is a central one with boundaries on either side of the median which can serve as an average group. In a Normal distribution the boundaries of the quintiles have boundaries ±0.253*s and ±0.842*s on either side of the mean (or median),where s is the sample standard deviation. Note that in a Normal distribution the mean, median and mode coincide.

Other frequently used quantiles are the deciles (10 equal sections) and the percentiles (100 equal sections)

# Averages

An average is simply a number that is representative of data. More particularly, it is a measure of central tendency. There are several types of average. Averages are useful for comparing data, especially when sets of different size are being compared.

Perhaps the simplest and commonly used average the arithmetic mean or more simply mean which is explained in the next section.

Other common types of average are the median, the mode, the geometric mean, and the harmonic mean, each of which may be the most appropriate one to use under different circumstances.

# Mean, Median, and Mode

## Mean, Median and Mode

### Mean

The mean, or more precisely the arithmetic mean, is simply the arithmetic average of a group of numbers (or data set) and is shown using -bar symbol $\bar {}$. So the mean of the variable x is $\bar{x}$, pronounced "x-bar". It is calculated by adding up all of the values in a data set and dividing by the number of values in that data set

$\bar x={\sum_{}x\over n}$.

For example, take the following set of data: {1,2,3,4,5}. The mean of this data would be:

$\bar x={\sum_{}x\over n}={1+2+3+4+5 \over 5}={15 \over 5}=3$

Here is a more complicated data set: {10,14,86,2,68,99,1}. The mean would be calculated like this:

$\bar x={\sum_{}x\over n}={10+14+86+2+68+99+1 \over 7}={280 \over 7}=40$

### Median

The median is the "middle value" in a set. That is, the median is the number in the center of a data set that has been ordered sequentially.

For example, let's look at the data in our second data set from above: {10,14,86,2,68,99,1}. What is its median?

• First, we sort our data set sequentially: {1,2,10,14,68,85,99}
• Next, we determine the total number of points in our data set (in this case, 7.)
• Finally, we determine the central position of or data set (in this case, the 4th position), and the number in the central position is our median - {1,2,10,14,68,85,99}, making 14 our median.
An easy way to determine the central position or positions for any ordered set is to take the total number of points, add 1, and then divide by 2. If the number you get is a whole number, then that is the central position. If the number you get is a fraction, take the two whole numbers on either side.

Because our data set had an odd number of points, determining the central position was easy - it will have the same number of points before it as after it. But what if our data set has an even number of points?

Let's take the same data set, but add a new number to it: {1,2,10,14,68,85,99,100} What is the median of this set?

When you have an even number of points, you must determine the two central positions of the data set. (See side box for instructions.) So for a set of 8 numbers, we get (8 + 1) / 2 = 9 / 2 = 4 1/2, which has 4 and 5 on either side.

Looking at our data set, we see that the 4th and 5th numbers are 14 and 68. From there, we return to our trusty friend the mean to determine the median. (14 + 68) / 2 = 82 / 2 = 41.

### Mode

The mode is the most common or "most frequent" value in a set. In the set {1, 2, 3, 4, 4, 4, 5, 6, 7, 8, 8, 9}, the mode would be 4 as it occurs a total of three times in the set, more frequently than any other value in the set.

A data set can have more than one mode: for example, in the set {1, 2, 2, 3, 3}, both 2 and 3 are modes. If all points in a data set occur with equal frequency, it is equally accurate to describe the data set as having many modes or no mode.

### Relationship of the Mean, Median, and Mode

The relationship of the mean, median, and mode to each other can provide some information about the relative shape of the data distribution. If the mean, median, and mode are approximately equal to each other, the distribution can be assumed to be approximately symmetrical. If the mean > median > mode, the distribution will be skewed to the right or positively skewed. If the mean < median < mode, the distribution will be skewed to the left or negatively skewed.

## Questions

1. There is an old joke that states: "Using median size as a reference it's perfectly possible to fit four ping-pong balls and two blue whales in a rowboat." Explain why this statement is true.

# Geometric Mean

## Geometric Mean

The Geometric Mean is calculated by taking the nth root of the product of a set of data.

$\tilde{x}=\sqrt[n\;]{\prod_{i=1}^n x_i}$

For example, if the set of data was:

1,2,3,4,5

The geometric mean would be calculated:

$\sqrt[5]{ 1 \times 2 \times 3 \times 4 \times 5} = \sqrt[5]{120} = 2.61$

Of course, with large n this can be difficult to calculate. Taking advantage of two properties of the logarithm:

$\log(a\cdot b) = \log(a) + \log(b)$

$\log( a^n ) = n \cdot \log( a )$

We find that by taking the logarithmic transformation of the geometric mean, we get:

$\log\left(\sqrt[n]{ x_1 \times x_2 \times x_3 \cdots x_n}\right) = \frac{1}{n} \sum_{i=1}^n\log(x_i)$

Which leads us to the equation for the geometric mean:

$\tilde{x}= \exp \left( \frac{1}{n} \sum_{i=1}^n\log(x_i) \right)$

## When to use the geometric mean

The arithmetic mean is relevant any time several quantities add together to produce a total. The arithmetic mean answers the question, "if all the quantities had the same value, what would that value have to be in order to achieve the same total?"

In the same way, the geometric mean is relevant any time several quantities multiply together to produce a product. The geometric mean answers the question, "if all the quantities had the same value, what would that value have to be in order to achieve the same product?"

For example, suppose you have an investment which returns 10% the first year, 50% the second year, and 30% the third year. What is its average rate of return? It is not the arithmetic mean, because what these numbers mean is that on the first year your investment was multiplied (not added to) by 1.10, on the second year it was multiplied by 1.50, and the third year it was multiplied by 1.30. The relevant quantity is the geometric mean of these three numbers.

It is known that the geometric mean is always less than or equal to the arithmetic mean (equality holding only when A=B). The proof of this is quite short and follows from the fact that $(\sqrt(A)-\sqrt(B))^2$ is always a non-negative number. This inequality can be surprisingly powerful though and comes up from time to time in the proofs of theorems in calculus. Source.

# Harmonic Mean

The arithmetic mean cannot be used when we want to average quantities such as speed.

Consider the example below:

Example 1: The distance from my house to town is 40 km. I drove to town at a speed of 40 km per hour and returned home at a speed of 80 km per hour. What was my average speed for the whole trip?.

Solution: If we just took the arithmetic mean of the two speeds I drove at, we would get 60 km per hour. This isn't the correct average speed, however: it ignores the fact that I drove at 40 km per hour for twice as long as I drove at 80 km per hour. To find the correct average speed, we must instead calcuate the harmonic mean.

For two quantities A and B, the harmonic mean is given by: $\frac{2}{\frac{1}{A} + \frac{1}{B}}$

This can be simplified by adding in the denominator and multiplying by the reciprocal: $\frac{2}{\frac{1}{A} + \frac{1}{B}} = \frac{2}{\frac{B + A}{AB}} = \frac{2AB}{A + B}$

For N quantities: A, B, C......

Harmonic mean = $\frac{N}{\frac{1}{A} + \frac{1}{B} + \frac{1}{C} + \ldots}$

Let us try out the formula above on our example:

Harmonic mean = $\frac{2AB}{A + B}$

Our values are A = 40, B = 80. Therefore, harmonic mean $= \frac{2 \times 40 \times 80}{40 + 80}= \frac{6400}{120} \approx 53.333$

Is this result correct? We can verify it. In the example above, the distance between the two towns is 40 km. So the trip from A to B at a speed of 40 km will take 1 hour. The trip from B to A at a speed to 80 km will take 0.5 hours. The total time taken for the round distance (80 km) will be 1.5 hours. The average speed will then be $\frac{80}{1.5} \approx$ 53.33 km/hour.

The harmonic mean also has physical significance.

# Relationships among Arithmetic, Geometric, and Harmonic Mean

The Means mentioned above are realizations of the generalized mean

$\bar{x}(m) = \left ( \frac{1}{n}\cdot\sum_{i=1}^n{|x_i|^m} \right ) ^{1/m}$

and ordered this way: $Minimum=\bar{x}(-\infty) < harmonic Mean=\bar{x}(-1) < geometric Mean=\bar{x}(0) < arithmetic Mean=\bar{x}(1) < Maximum=\bar{x}(\infty)$

# Moving Average

A moving average is used when you want to get a general picture of the trends contained in a data set. The data set of concern is typically a so-called "time series", i.e a set of observations ordered in time. Given such a data set X, with individual data points xi, a 2n+1 point moving average is defined as $\bar{x_{i}}=\frac{1}{2n+1}\sum_{k=i-n}^{i+n}x_{k}$, and is thus given by taking the average of the 2n points around xi. Doing this on all data points in the set (except the points too close to the edges) generates a new time series that is somewhat smoothed, revealing only the general tendencies of the first time series.

The moving average for many time-based observations is often lagged. That is, we take the 10 -day moving average by looking at the average of the last 10 days. We can make this more exciting (who knew statistics was exciting?) by considering different weights on the 10 days. Perhaps the most recent day should be the most important in our estimate and the value from 10 days ago would be the least important. As long as we have a set of weights that sums to 1, this is an acceptable moving-average. Sometimes the weights are chosen along an exponential curve to make the exponential moving-average.

# Variance and Standard Deviation

Probability density function for the normal distribution. The green line is the standard normal distribution.

## Measure of Scale

When describing data it is helpful (and in some cases necessary) to determine the spread of a distribution. One way of measuring this spread is by calculating the variance or the standard deviation of the data.

In describing a complete population, the data represents all the elements of the population. As a measure of the "spread" in the population one wants to know a measure of the possible distances between the data and the population mean. There are several options to do so. One is to measure the average absolute value of the deviations. Another, called the variance, measures the average square of these deviations.

A clear distinction should be made between dealing with the population or with a sample from it. When dealing with the complete population the (population) variance is a constant, a parameter which helps to describe the population. When dealing with a sample from the population the (sample) variance is actually a random variable, whose value differs from sample to sample. Its value is only of interest as an estimate for the population variance.

### Population variance and standard deviation

Let the population consists of the N elements x1,...,xN. The (population) mean is:

$\mu = \frac 1N \sum_{i=1}^Nx_i$.

The (population) variance σ2 is the average of the squared deviations from the mean or (xi - μ)2 - the square of the value's distance from the distribution's mean.

$\sigma^2 = \frac 1N \sum_{i=1}^N (x_i - \mu)^2$.

Because of the squaring the variance is not directly comparable with the mean and the data themselves. The square root of the variance is called the Standard Deviation σ. Note that σ is the root mean squared of differences between the data points and the average.

### Sample variance and standard deviation

Let the sample consist of the n elements x1,...,xn, taken from the population. The (sample) mean is:

$\bar{x} = \frac 1n \sum_{i=1}^nx_i$.

The sample mean serves as an estimate for the population mean μ.

The (sample) variance s2 is a kind of average of the squared deviations from the (sample) mean:

$s^2 = \frac 1{n-1} \sum_{i=1}^n (x_i - \bar{x})^2$.

Also for the sample we take the square root to obtain the (sample) standard deviation s

A common question at this point is "why do we square the numerator?" One answer is: to get rid of the negative signs. Numbers are going to fall above and below the mean and, since the variance is looking for distance, it would be counterproductive if those distances factored each other out.

## Example

When rolling a fair die, the population consists of the 6 possible outcomes 1 to 6. A sample may consist instead of the outcomes of 1000 rolls of the die.

The population mean is:

$\mu = \frac 16 (1+2+3+4+5+6) = 3.5$,

and the population variance:

$\sigma^2=\frac 16 \sum_{i=1}^n (i-3.5)^2=\frac 16(6.25+2.25+0.25+0.25+2.25+6.25)=\frac {35}{12} \approx 2.917$

The population standard deviation is:

$\sigma = \sqrt{\frac {35}{12}} \approx 1.708$.

Notice how this standard deviation is somewhere in between the possible deviations.

So if we were working with one six-sided die: X = {1, 2, 3, 4, 5, 6}, then σ2 = 2.917. We will talk more about why this is different later on, but for the moment assume that you should use the equation for the sample variance unless you see something that would indicate otherwise.

Note that none of the above formulae are ideal when calculating the estimate and they all introduce rounding errors. Specialized statistical software packages use more complicated logarithms that take a second pass of the data in order to correct for these errors. Therefore, if it matters that your estimate of standard deviation is accurate, specialized software should be used. If you are using non-specialized software, such as some popular spreadsheet packages, you should find out how the software does the calculations and not just assume that a sophisticated algorithm has been implemented.

### For Normal Distributions

The empirical rule states that approximately 68 percent of the data in a normally distributed dataset is contained within one standard deviation of the mean, approximately 95 percent of the data is contained within 2 standard deviations, and approximately 99.7 percent of the data falls within 3 standard deviations.

As an example, the verbal or math portion of the SAT has a mean of 500 and a standard deviation of 100. This means that 68% of test-takers scored between 400 and 600, 95% of test takers scored between 300 and 700, and 99.7% of test-takers scored between 200 and 800 assuming a completely normal distribution (which isn't quite the case, but it makes a good approximation).

## Robust Estimators

For a normal distribution the relationship between the standard deviation and the interquartile range is roughly: SD = IQR/1.35.

For data that are non-normal, the standard deviation can be a terrible estimator of scale. For example, in the presence of a single outlier, the standard deviation can grossly overestimate the variability of the data. The result is that confidence intervals are too wide and hypothesis tests lack power. In some (or most) fields, it is uncommon for data to be normally distributed and outliers are common.

One robust estimator of scale is the "average absolute deviation", or aad. As the name implies, the mean of the absolute deviations about some estimate of location is used. This method of estimation of scale has the advantage that the contribution of outliers is not squared, as it is in the standard deviation, and therefore outliers contribute less to the estimate. This method has the disadvantage that a single large outlier can completely overwhelm the estimate of scale and give a misleading description of the spread of the data.

Another robust estimator of scale is the "median absolute deviation", or mad. As the name implies, the estimate is calculated as the median of the absolute deviation from an estimate of location. Often, the median of the data is used as the estimate of location, but it is not necessary that this be so. Note that if the data are non-normal, the mean is unlikely to be a good estimate of location.

It is necessary to scale both of these estimators in order for them to be comparable with the standard deviation when the data are normally distributed. It is typical for the terms aad and mad to be used to refer to the scaled version. The unscaled versions are rarely used.

# Displaying Data

A single statistic tells only part of a dataset’s story. The mean is one perspective; the median yet another. And when we explore relationships between multiple variables, even more statistics arise. The coefficient estimates in a regression model, the Cochran-Maentel-Haenszel test statistic in partial contingency tables; a multitude of statistics are available to summarize and test data.

But our ultimate goal in statistics is not to summarize the data, it is to fully understand their complex relationships. A well designed statistical graphic helps us explore, and perhaps understand, these relationships.

This section will help you let the data speak, so that the world may know its story.

• [1] "Show me the Numbers" by Stephen Few has a less technical approach to creating graphics. You might want to scan through this book if you are building a library on making graphs.

# Bar Charts

The Bar Chart (or Bar Graph) is one of the most common ways of displaying catagorical/qualitative data. Bar Graphs consist of 2 variables, one response (sometimes called "dependent") and one predictor (sometimes called "independent"), arranged on the horizontal and vertical axis of a graph. The relationship of the predictor and response variables is shown by a mark of some sort (usually a rectangular box) from one variable's value to the other's.

To demonstrate we will use the following data(tbl. 3.1.1) representing a hypothetical relationship between a qualitative predictor variable, "Graph Type", and a quantitative response variable, "Votes".

tbl. 3.1.1 - Favourite Graphs

Bar Charts 5
Pie Graphs 2
Histograms 3
Pictograms 8
Comp. Pie Graphs 4
Line Graphs 9
Frequency Polygon 1
Scatter Graphs 5

From this data we can now construct an appropriate graphical representation which, in this case will be a Bar Chart. The graph may be orientated in several ways, of which the vertical chart (fig. 3.1.1) is most common, with the horizontal chart(fig. 3.1.2) also being used often

fig. 3.1.1 - vertical chart

fig. 3.1.2 - horizontal chart

Take note that the height and width of the bars, in the vertical and horizontal Charts, respectfully, are equal to the response variable's corresponding value - "Bar Chart" bar equals the number of votes that the Bar Chart type received in tbl. 3.1.1

Also take note that there is a pronounced amount of space between the individual bars in each of the graphs, this is important in that it help differentiate the Bar Chart graph type from the Histogram graph type discussed in a later section.

# Histograms

## Histograms

File:Morley.png

It is often useful to look at the distribution of the data, or the frequency with which certain values fall between pre-set bins of specified sizes. The selection of these bins is up to you, but remember that they should be selected in order to illuminate your data, not obfuscate it.

To produce a histogram:

• Select a minimum, a maximum, and a bin size. All three of these are up to you. In the Michaelson-Morley data used above the minimum is 600, the maximum is 1100, and the bin size is 50.
• Calculate your bins and how many values fall into each of them. For the Michaelson-Morley data the bins are:
• 600 ≤ x < 650, 2 values.
• 650 ≤ x < 700, 0 values.
• 700 ≤ x < 750, 7 values.
• 750 ≤ x < 800, 16 values.
• 800 ≤ x < 850, 30 values.
• 850 ≤ x < 900, 22 values.
• 900 ≤ x < 950, 11 values.
• 950 ≤ x < 1000, 11 values.
• 1000 ≤ x < 1050, 0 values.
• 1050 ≤ x < 1100, 1 value.
• Plot the counts you figured out above. Do this using a standard bar plot.

There! You are done. Now let's do an example.

### Worked Problem

Let's say you are an avid roleplayer who loves to play Mechwarrior, a d6 (6 sided die) based game. You have just purchased a new 6 sided die and would like to see whether it is biased (in combination with you when you roll it).

#### What We Expect

So before we look at what we get from rolling the die, let's look at what we would expect. First, if a die is unbiased it means that the odds of rolling a six are exactly the same as the odds of rolling a 1--there wouldn't be any favoritism towards certain values. Using the standard equation for the arithmetic mean find that μ = 3.5. We would also expect the histogram to be roughly even all of the way across--though it will almost never be perfect simply because we are dealing with an element of random chance.

#### What We Get

Here are the numbers that you collect:

 1 5 6 4 1 3 5 5 6 4 1 5 6 6 4 5 1 4 3 6 1 3 6 4 2 4 1 6 4 2 2 4 3 4 1 1 6 3 5 5 4 3 5 3 4 2 2 5 6 5 4 3 5 3 3 1 5 4 4 5 1 2 5 1 6 5 4 3 2 4 2 1 3 3 3 4 6 1 1 3 6 6 1 4 6 6 6 5 3 1 5 6 3 4 5 5 5 2 4 4

#### Analysis

$\bar{X} = 3.71$

Referring back to what we would expect for an unbiased die, this is pretty close to what we would expect. So let's create a histogram to see if there is any significant difference in the distribution.

The only logical way to divide up dice rolls into bins is by what's showing on the die face:

 1 2 3 4 5 6 16 9 17 21 20 17

If we are good at visualizing information, we can simple use a table, such as in the one above, to see what might be happening. Often, however, it is useful to have a visual representation. As the amount of variety of data we want to display increases, the need for graphs instead of a simple table increases.

Looking at the above figure, we clearly see that sides 1, 3, and 6 are almost exactly what we would expect by chance. Sides 4 and 5 are slightly greater, but not too much so, and side 2 is a lot less. This could be the result of chance, or it could represent an actual anomaly in the data and it is something to take note of keep in mind. We'll address this issue again in later chapters.

### Frequency Density

Another way of drawing a histogram is to work out the Frequency Density.

Frequency Density
The Frequency Density is the frequency divided by the class width.

The advantage of using frequency density in a histogram is that doesn't matter if there isn't an obvious standard width to use. For all the groups, you would work out the frequency divided by the class width for all of the groups.

Statistics

# Scatter Plots

Scatter Plot is used to show the relationship between 2 numeric variables. It is not useful when comparing discrete variables versus numeric variables. A scatter plot matrix is a collection of pairwise scatter plots of numeric variables.

# Box Plots

Figure 1. Box plot of data from the Michelson-Morley Experiment

A box plot (also called a box and whisker diagram) is a simple visual representation of key features of a univariate sample.

The box lies on a vertical axis in the range of the sample. Typically, a top to the box is placed at the 1st quartile, the bottom at the third quartile. The width of the box is arbitrary, as there is no x-axis (though see Violin Plots, below).

In between the top and bottom of the box is some representation of central tendency. A common version is to place a horizontal line at the median, dividing the box into two. Additionally, a star or asterisk is placed at the mean value, centered in the box in the horizontal direction.

Another common extension is to the 'box-and-whisker' plot. This adds vertical lines extending from the top and bottom of the plot to for example, the maximum and minimum values, The farthest value within 2 standard deviations above and below the mean. Alternatively, the whiskers could extend to the 2.5 and 97.5 percentiles. Finally, it is common in the box-and-whisker plot to show outliers (however defined) with asterisks at the individual values beyond the ends of the whiskers.

Violin Plots are an extension to box plots using the horizontal information to present more data. They show some estimate of the CDF instead of a box, though the quantiles of the distribution are still shown.

# Pie Charts

A pie chart showing the racial make-up of the US in 2000.
Pie chart of populations of English language-speaking people

A Pie-Chart/Diagram is a graphical device - a circular shape broken into sub-divisions. The sub-divisions are called "sectors", whose areas are proportional to the various parts into which the whole quantity is divided. The sectors may be coloured differently to show the relationship of parts to the whole. A pie diagram is an alternative of the sub-divided bar diagram.

To construct a pie-chart, first we draw a circle of any suitable radius then the whole quantity which is to be divided is equated to 360 degrees. The different parts of the circle in terms of angles are calculated by the following formula.

    Component Value / Whole Quantity * 360


The component parts i.e. sectors have been cut beginning from top in clockwise order.

Note that the percentages in a list may not add up to exactly 100% due to rounding. For example if a person spends a third of their time on each of three activities: 33%, 33% and 33% sums to 99%.

Warning: Pie charts are a very bad way of displaying information. The eye is good at judging linear measures and bad at judging relative areas. A bar chart or dot chart is a preferable way of displaying this type of data.

Cleveland (1985), page 264: "Data that can be shown by pie charts always can be shown by a dot chart. This means that judgements of position along a common scale can be made instead of the less accurate angle judgements." This statement is based on the empirical investigations of Cleveland and McGill as well as investigations by perceptual psychologists.

# Comparative Pie Charts

A pie chart showing preference of colors by two groups.

The comparative pie charts are very difficult to read and compare if the ratio of the pie chart is not given.

Examine our example of color preference for two different groups. How much work does it take to see that the Blue preference for both groups is the same? First, we have to find blue on each pie, and then remember how many degrees it has. If we did not include the share for blue in the label, then we would probably be approximating the comparison. So, if we use multiple pie charts, we have to expect that comparisions between charts would only be approximate.

What is the most popular color in the left graph? Red. But note, that you have to look at all of the colors and read the label to see which it might be. Also, this author was kind when creating these two graphs because I used the same color for the same object. Imagine the confusion if one had made the most important color get Red in the right-hand chart?

If two shares of data should not be compared via the comparative pie chart, what kind of graph would be preferred? The stacked bar chart is probably the most appropriate for sharing of the total comparisons. Again, exact comparisons cannot be done with graphs and therefore a table may supplement the graph with detailed information.

# Pictograms

A pictogram is simply a picture that conveys some statistical information. A very common example is the thermometer graph so common in fund drives. The entire thermometer is the goal (number of dollars that the fund raisers wish to collect. The red stripe (the "mercury") represents the proportion of the goal that has already been collected.

Another example is a picture that represents the gender constitution of a group. Each small picture of a male figure might represent 1,000 men and each small picture of a female figure would, then, represent 1,000 women. A picture consisting of 3 male figures and 4 female figures would indicate that the group is made up of 3,000 men and 4,000 women.

An interesting pictograph is the Chernoff Faces. It is useful for displaying information on cases for which several variables have been recorded. In this kind of plot, each case is represented by a separate picture of a face. The sizes of the various features of each face are used to present the value of each variable. For instance, if blood pressure, high density cholesterol, low density cholesterol, body temperature, height, and weight are recorded for 25 individuals, 25 faces would be displayed. The size of the nose on each face would represent the level of that person's blood pressure. The size of the left eye may represent the level of low density cholesterol while the size of the right eye might represent the level of high density cholesterol. The length of the mouth could represent the person's temperature. The length of the left ear might indicate the person's height and that of the right ear might represent their weight. Of course, a legend would be provided to help the viewer determine what feature relates to which variable. Where it would be difficult to represent the relationship of all 6 variables on a single (6-dimensional) graph, the Chernoff Faces would give a relatively easy to interpret 6-dimensional representation.

# Line Graphs

Basically, a line graph can be, for example, a picture of what happened by/to something (a variable) during a specific time period (also a variable).

On the left side of such a graph usually is as an indication of that "something" in the form of a scale, and at the bottom is an indication of the specific time involved.

Usually a line graph is plotted after a table has been provided showing the relationship between the two variables in the form of pairs. Just as in (x,y) graphs, each of the pairs results in a specific point on the graph, and being a LINE graph these points are connected to one another by a LINE.

Many other line graphs exist; they all CONNECT the points by LINEs, not necessarily straight lines. Sometimes polynomials, for example, are used to describe approximately the basic relationship between the given pairs of variables, and between these points. The higher the degree of the polynomial, the more accurate is the "picture" of that relationship, but the degree of that polynomial must never be higher than n-1, where n is the number of the given points.

Graph theory

[[../../Curve fitting|Curve fitting]]

From Wikipedia: Line graph and Curve fitting

# Frequency Polygon

This is a histogram with an overlaid frequency polygon.

A frequency polygon shows approximately the smooth curve that would describe a frequency distribution if the class intervals were made as small as possible and the number of observations were very large. The very common bell curve used to represent a normal distribution is an idealized, smoothed frequency polygon.

One way to form a frequency polygon is to connect the midpoints at the top of the bars of a histogram with line segments (or a smooth curve). Of course the midpoints themselves could easily be plotted without the histogram and be joined by line segments. Sometimes it is beneficial to show the histogram and frequency polygon together.

Unlike histograms, frequency polygons can be superimposed so as to compare several frequency distributions.

# Introduction to Probability

When throwing two dice, what is the probability that their sum equals seven?

## Introduction to probability

### Why have probability in a statistics textbook?

Very little in mathematics is truly self contained. Many branches of mathematics touch and interact with one another, and the fields of probability and statistics are no different. A basic understanding of probability is vital in grasping basic statistics, and probability is largely abstract without statistics to determine the "real world" probabilities.

This section is not meant to give a comprehensive lecture in probability, but rather simply touch on the basics that are needed for this class, covering the basics of Bayesian Analysis for those students who are looking for something a little more interesting. This knowledge will be invaluable in attempting to understand the mathematics involved in various Distributions that come later.

### Set notion

A set is a collection of objects. We usually use capital letters to denote sets, for e.g., A is the set of females in this room.

• The members of a set A are called the elements of A. For e.g., Patricia is an element of A (Patricia ∈ A) Patrick is not an element of A (Patrick ∉ A).

• The universal set, U, is the set of all objects under consideration. For e.g., U is the set of all people in this room.

• The null set or empty set, ∅, has no elements. For e.g., the set of males above 2.8m tall in this room is an empty set.

• The complement Ac of a set A is the set of elements in U outside A. I.e. x ∈ Ac iff x ∉ A.

• Let A and B be 2 sets. A is a subset of B if each element of A is also an element of B. Write A ⊂ B. For e.g., The set of females wearing metal frame glasses in this room ⊂ the set of females wearing glasses in this room ⊂ the set of females in this room.

• The intersection A ∩ B of two sets A and B is the set of the common elements. I.e. x ∈ A ∩ B iff x ∈ A and x ∈ B.

• The union A ∪ B of two sets A and B is the set of all elements from A or B. I.e. x ∈ A ∪ B iff x ∈ A or x ∈ B.

A Venn diagram.

## Probability

Probability is connected with some unpredictability. We know what outcomes may occur, but not exactly which one. The set of possible outcomes plays a basic role. We call it the sample space and indicate it by S. Elements of S are called outcomes. In rolling a dice the sample space is S = {1,2,3,4,5,6}. Not only do we speak of the outcomes, but also about events, sets of outcomes. E.g. in rolling a dice we can ask whether the outcome was an even number, which means asking after the event "even" = E = {2,4,6}. In simple situations with a finite number of outcomes, we assign to each outcome s (∈ S) its probability (of occurrence) p(s) (written with a small p), a number between 0 and 1. It is a quite simple function, called the probability function, with the only further property that the total of all the probabilities sum up to 1. Also for events A do we speak of their probability P(A) (written with a capital P), which is simply the total of the probabilities of the outcomes in A. For a fair dice p(s) = 1/6 for each outcome s and P("even") = P(E) = 1/6+1/6+1/6 = 1/2.

The general concept of probability for non-finite sample spaces is a little more complex, although it rests on the same ideas.

### Negation

Negation is a way of saying "not A", hence saying that the complement of A has occurred. For example: "What is the probability that a six-sided die will not land on a one?" (five out of six, or p = 0.833)

P[X'] = 1 - P[X]

Or, more colloquially, "the probability of 'not X' together with the probability of 'X' equals one or 100%."

# Bernoulli Trials

A lot of experiments just have two possible outcomes, generally referred to as "success" and "failure". If such an experiment is independently repeated we call them (a series of) Bernoulli trials. Usually the probability of success is called p. The repetition may be done in several ways:

• a fixed number of times (n); as a consequence the observed number of successes is stochastic;
• until a fixed number of successes (m) is observed; as a consequence the number experiments is stochastic;

In the first case the number of successes is Binomial distributed with parameters n and p. For n=1 the distribution is also called the Bernoulli distribution. In the second case the number of experiments is Negative Binomial distributed with parameters m and p. For m=1 the distribution is also called the Geometric distribution.

# Introductory Bayesian Analysis

Bayesian analysis is the branch of statistics based on the idea that we have some knowledge in advance about the probabilities that we are interested in, so called a priori probabilities. This might be your degree of belief in a particular event, the results from previous studies, or a general agreed-upon starting value for a probability. The terminology "Bayesian" comes from the Bayesian rule or law, a law about conditional probabilities. The opposite of "Bayesian" is sometimes referred to as "Classical Statistics."

### Example

Consider a box with 3 coins, with probabilities of showing heads respectively 1/4, 1/2 and 3/4. We choose arbitrarily one of the coins. Hence we take 1/3 as the a priori probability P(C1) of having chosen coin number 1. After 5 throws, in which X=4 times heads came up, it seems less likely that the coin is coin number 1. We calculate the a posteriori probability that the coin is coin number 1, as:

$P(C_1|X=4)=\frac{P(X=4|C_1)P(C_1)}{P(X=4)}=\frac{P(X=4|C_1)P(C_1)}{P(X=4|C_1)+P(X=4|C_2)+P(X=4|C_3)}= \frac{ {5 \choose 4} (\frac 14)^4 \frac 34 \frac 13} {{5 \choose 4} (\frac 14)^4 \frac 34 \frac 13+{5 \choose 4} (\frac 12)^4 \frac 12 \frac 13+{5 \choose 4} (\frac 34)^4 \frac 14 \frac 13}=$

In words:

The probability that the Coin is the first Coin, given that we know heads came up 4 times... Is equal to the probability that heads came up 4 times given we know it's the first coin, times the probability that the coin is the first coin. All divided by the probability that heads comes up 4 times (ignoring which of the three Coins is chosen). The binomial coefficients cancel out as well as all denominators when expanding 1/2 to 2/4. This results in
$\frac{3}{3 + 32 + 81}=\frac{3}{116}$

In the same way we find:

$P(C_2|X=4)=\frac{32}{3 + 32 + 81}=\frac{32}{116}$

and

$P(C_3|X=4)=\frac{81}{3 + 32 + 81}=\frac{81}{116}$.

This shows us that after examining the outcome of the five throws, it is most likely we did choose coin number 3.

Actually for a given result the denominator does not matter, only the relative Probabilities p(Ci) = P(Ci | X = 4) / P(X = 4) When the result is 3 times heads the Probabilities change in favor of Coin 2 and further as the following table shows:

5 1 32 243
4 3 32 81
3 9 32 27
2 27 32 9
1 81 32 3
0 243 32 1

# Distributions

How are the results of the latest SAT test? What is the average height of females under 21 in Zambia? How does beer consumption among college students at engineering college compare to college students in liberal arts colleges?

To answer these questions, we would collect data and put them in a form that is easy to summarize, visualize, and discuss. Loosely speaking, the collection and aggregation of data result in a distribution. Distributions are most often in the form of a histogram or a table. That way, we can "see" the data immediately and begin our scientific inquiry.

For example, if we want to know more about students' latest performance on the SAT, we would collect SAT scores from ETS, compile them in a way that is pertinent to us, and then form a distribution of these scores. The result may be a data table or it may be a plot. Regardless, once we "see" the data, we can begin asking more interesting research questions about our data.

The distributions we create often parallel distributions that are mathematically generated. For example, if we obtain the heights of all high school students and plot this data, the graph may resemble a normal distribution, which is generated mathematically. Then, instead of painstakingly collecting heights of all high school students, we could simply use a normal distribution to approximate the heights without sacrificing too much accuracy.

In the study of statistics, we focus on mathematical distributions for the sake of simplicity and relevance to the real-world. Understanding these distributions will enable us to visualize the data easier and build models quicker. However, they cannot and do not replace the work of manual data collection and generating the actual data distribution.

What percentage lie within a certain range? Distributions show what percentage of the data lies within a certain range. So, given a distribution, and a set of values, we can determine the probability that the data will lie within a certain range.

The same data may lead to different conclusions if it is interposed on different distributions. So, it is vital in all statistical analysis for data to be put onto the correct distribution.

# Discrete Distributions

'Discrete' data are data that assume certain discrete and quantized values. For example, true-false answers are discrete, because there are only two possible choices. Valve settings such as 'high/medium/low' can be considered as discrete values. As a general rule, if data can be counted in a practical manner, then they can be considered to be discrete.

To demonstrate this, let us consider the population of the world. It is a discrete number because the number of civilians is theoretically countable. But since this is not practicable, statisticians often treat this data as continuous. That is, we think of population as within a range of numbers rather than a single point.

For the curious, the world population is 6,533,596,139 as of August 9, 2006. Please note that statisticians did not arrive at this figure by counting individual residents. They used much smaller samples of the population to estimate the whole. Going back to Chapter 1, this is a great reason to learn statistics - we need only a smaller sample of data to make intelligent descriptions of the entire population!

Discrete distributions result from plotting the frequency distribution of data which is discrete in nature.

## Cumulative Distribution Function

A discrete random variable has a cumulative distribution function that describes the probability that the random variable is below the point. The cumulative distribution must increase towards 1. Depending on the random variable, it may reach one at a finite number, or it may not. The cdf is represented by a capital F.

## Probability Mass Function

A discrete random variable has a probability mass function that describes how likely the random variable is to be at a certain point. The probability mass function must have a total of 1, and sums to the cdf. The pmf is represented by the lowercase f.

## Special Values

The expected value of a discrete variable is $\sum_{n_{min}}^{n_{max}} x_i f(x_i)$

The expected value of any function of a discrete variable g(X) is $\sum_{n_{min}}^{n_{max}} g(x_i)f(x_i)$

The variance is equal to E((XE(X))2)

Simulating binomial, hypergeometric, and the Poisson distribution: Discrete Distributions

# Bernoulli Distribution

## Bernoulli Distribution: The coin toss

There is no more basic random event than the flipping of a coin. Heads or tails. It's as simple as you can get! The "Bernoulli Trial" refers to a single event which can have one of two possible outcomes with a fixed probability of each occurring. You can describe these events as "yes or no" questions. For example:

• Will the coin land heads?
• Will the newborn child be a girl?
• Are a random person's eyes green?
• Will a mosquito die after the area was sprayed with insecticide?
• Will a potential customer decide to buy my product?
• Will a citizen vote for a specific candidate?
• Is an employee going to vote pro-union?
• Will this person be abducted by aliens in their lifetime?

The Bernoulli Distribution has one controlling parameter: the probability of success. A "fair coin" or an experiment where success and failure are equally likely will have a probability of 0.5 (50%). Typically the variable p is used to represent this parameter.

If a random variable X is distributed with a Bernoulli Distribution with a parameter p we write its probability mass function as:

$f_X(x) = \begin{cases}p, & \mbox{if } x = 1\\1-p, & \mbox{if } x = 0\end{cases}$

Where the event X=1 represents the "yes."

This distribution may seem trivial, but it is still a very important building block in probability. The Binomial distribution extends the Bernoulli distribution to encompass multiple "yes" or "no" cases with a fixed probability. Take a close look at the examples cited above. Some similar questions will be presented in the next section which might give an understanding of how these distributions are related.

# Binomial Distribution

## Binomial Distribution

Where the Bernoulli Distribution asks the question of "Will this single event succeed?" the Binomial is associated with the question "Out of a given number of trials, how many will succeed?" Some example questions that are modeled with a Binomial distribution are:

• Out of ten tosses, how many times will this coin land heads?
• From the children born in a given hospital on a given day, how many of them will be girls?
• How many students in a given classroom will have green eyes?
• How many mosquitos, out of a swarm, will die when sprayed with insecticide?

The relation between the Bernoulli and Binomial distributions is intuitive: The Binomial distribution is composed of multiple Bernoulli trials. We conduct n repeated experiments where the probability of success is given by the parameter p and add up the number of successes. This number of successes is represented by the random variable X. The value of X is then between 0 and n.

When a random variable X has a Binomial Distribution with parameters p and n we write it as X ~ Bin(n,p) or X ~ B(n,p) and the probability mass function is given by the equation:

$P\left[X = k\right] = \begin{cases} {n \choose k} p^k \left(1-p\right)^{n-k}\ & 0 \le k \le n \\ 0 & \mbox{otherwise} \end{cases}$

where ${n \choose k}={n! \over k!(n-k)!}$

For a refresher on factorials (n!), go back to the Refresher Course earlier in this wiki book.

### An example

Let's walk through a simple example of the Binomial distribution. We're going to use some pretty small numbers because factorials can be hard to compute. (Few basic calculators even feature them!) We are going to ask five random people if they believe there is life on other planets. We are going to assume in this example that we know 30% of people believe this to be true. We want to ask the question: "How many people will say they believe in extraterrestrial life?" Actually, we want to be more specific than that: "What is the probability that exactly 2 people will say they believe in extraterrestrial life?"

We know all the values that we need to plug into the equation. The number of people asked, n=5. The probability of any given person answering "yes", p=0.3. (Remember, I said that 30% of people believe in life on other planets!) Finally, we're asking for the probability that exactly 2 people answer "yes" so k=2. This yields the equation:

$P \left[X = 2 \right] = {5 \choose 2} \cdot {{0.3^2 \cdot} {\left( 1 - 0.3 \right)^{3}}} = {10} \cdot {{0.3^2} \cdot {\left( 1-0.3 \right)^{3}}} = 0.3087$ since ${5 \choose 2}={5! \over 2! \cdot 3!}={5 \cdot 4 \cdot 3 \cdot 2 \cdot 1 \over (2 \cdot 1) \cdot (3 \cdot 2 \cdot 1)}={120 \over 12}=10$

Here are the probabilities for all the possible values of X. You can get these values by replacing the k=2 in the above equation with all values from 0 to 5.

 Value for k Probability f(k) 0 0.16807 1 0.36015 2 0.30870 3 0.13230 4 0.02835 5 0.00243

What can we learn from these results? Well, first of all we'll see that it's just a little more likely that only one person will confess to believing in life on other planets. There's a distinct chance (about 17%) that nobody will believe it, and there's only a 0.24% (a little over 2 in 1000) that all five people will be believers.

### Explanation of the equation

Take the above example. Let's consider each of the five people one by one.

The probability that any one person believes in extraterrestrial life is 30%, or 0.3. So the probability that any two people both believe in extraterrestrial life is 0.3 squared. Similarly, the probability that any one person does not believe in extraterrestrial life is 70%, or 0.7, so the probability that any three people do not believe in extraterrestrial life is 0.7 cubed.

Now, for two out of five people to believe in extraterrestrial life, two conditions must be satisfied: two people believe in extraterrestrial life, and three do not. The probability of two out of five people believing in extraterrestrial life would thus appear to be 0.3 squared (two believers) times 0.7 cubed (three non-believers), or 0.03087.

However, in doing this, we are only considering the case whereby the first two selected people are believers. How do we consider cases such as that in which the third and fifth people are believers, which would also mean a total of two believers out of five?

The answer lies in combinatorics. Bearing in mind that the probability that the first two out of five people believe in extraterrestrial life is 0.03087, we note that there are C(5,2), or 10, ways of selecting a set of two people from out of a set of five, i.e. there are ten ways of considering two people out of the five to be the "first two". This is why we multiply by C(n,k). The probability of having any two of the five people be believers is ten times 0.03087, or 0.3087.

# Poisson Distribution

## Poisson Distribution

Any French speaker will notice that "Poisson" means "fish", but really there's nothing fishy about this distribution. It's actually pretty straightforward. The name comes from the mathematician Siméon-Denis Poisson (1781-1840).

The Poisson Distribution is very similar to the Binomial Distribution. We are examining the number of times an event happens. The difference is subtle. Whereas the Binomial Distribution looks at how many times we register a success over a fixed total number of trials, the Poisson Distribution measures how many times a discete event occurs, over a period of continuous space or time. There isn't a "total" value n. As with the previous sections, let's examine a couple of experiments or questions that might have an underlying Poisson nature.

• How many pennies will I encounter on my walk home?
• How many children will be delivered at the hospital today?
• How many mosquito bites did you get today after having sprayed with insecticide?
• How many angry phone calls did I get after airing a particularly distasteful political ad?
• How many products will I sell after airing a new television commercial?
• How many people, per hour, will cross a picket line into my store?
• How many alien abduction reports will be filed this year?
• How many defects will there be per 100 metres of rope sold?

What's a little different about this distribution is that the random variable X which counts the number of events can take on any non-negative integer value. In other words, I could walk home and find no pennies on the street. I could also find one penny. It's also possible (although unlikely, short of an armored-car exploding nearby) that I would find 10 or 100 or 10,000 pennies.

Instead of having a parameter p that represents a component probability like in the Bernoulli and Binomial distributions, this time we have the parameter "lambda" or λ which represents the "average or expected" number of events to happen within our experiment. The probability mass function of the Poisson is given by

$P(N=k)=\frac{e^{-\lambda}\lambda^k}{k!}$.

### An example

We run a restaurant and our signature dish (which is very expensive) gets ordered on average 4 times per day. What is the probability of having this dish ordered exactly 3 times tomorrow? If we only have the ingredients to prepare 3 of these dishes, what is the probability that it will get sold out and we'll have to turn some orders away?

The probability of having the dish ordered 3 times exactly is given if we set k=3 in the above equation. Remember that we've already determined that we sell on average 4 dishes per day, so λ=4.

$P(N=k)=\frac{e^{-\lambda}\lambda^k}{k!} = \frac{e^{-4} 4^3}{3!} = 0.195$

Here's a table of the probabilities for all values from k=0..6:

 Value for k Probability f(k) 0 0.0183 1 0.0733 2 0.1465 3 0.1954 4 0.1954 5 0.1563 6 0.1042

Now for the big question: Will we run out of food by the end of the day tomorrow? In other words, we're asking if the random variable X>3. In order to compute this we would have to add the probabilities that X=4, X=5, X=6,... all the way to infinity! But wait, there's a better way!

The probability that we run out of food P(X>3) is the same as 1 minus the probability that we don't run out of food, or 1-P(X≤3). So if we total the probability that we sell zero, one, two and three dishes and subtract that from 1, we'll have our answer. So,

1 - P(X≤3) = 1 - ( P(X=0) + P(X=1) + P(X=2) + P(X=3) ) = 1 - 0.4335 = 0.5665

In other words, we have a 56.65% chance of selling out of our wonderful signature dish. I guess crossing our fingers is in order!

# Geometric Distribution

Geometric Distribution refers to the probability of the number of times needed to do something until getting a desired result. For example:

• How many times will I throw a coin until it lands on heads?
• How many children will I have until I get a girl?
• How many cards will I draw from a pack until I get a Joker?

Just like the Bernoulli Distribution, the Geometric distribution has one controling parameter: The probability of success in any independent test.

If a random variable X is distributed with a Geometric Distribution with a parameter p we write its probability mass function as:

$P\left( X=i \right) =p\left( 1-p\right)^{i-1}$

With a Geometric Distribution it is also pretty easy to calculate the probability of a "more than n times" case. The probability of failing to achieve the wanted result is $\left( 1-p\right)^k$.

Example: a student comes home from a party in the forest, in which interesting substances were consumed. The student is trying to find the key to his front door, out of a keychain with 10 different keys. What is the probability of the student succeeding in finding the right key in the 4th attempt?

$P\left( X=4 \right) =\frac{1}{10}\left( 1-\frac{1}{10}\right)^{4-1}=\frac{1}{10}\left( \frac{9}{10}\right)^{3}=0.0729$

# Negative Binomial Distribution

Just as the Bernoulli and the Binomial distribution are related in counting the number of successes in 1 or more trials, the Geometric and the Negative Binomial distribution are related in the number of trials needed to get 1 or more successes.

The Negative Binomial distribution refers to the probability of the number of times needed to do something until achieving a fixed number of desired results. For example:

• How many times will I throw a coin until it lands on heads for the 10th time?
• How many children will I have when I get my third daughter?
• How many cards will I have to draw from a pack until I get the second Joker?

Just like the Binomial Distribution, the Negative Binomial distribution has two controlling parameters: the probability of success p in any independent test and the desired number of successes m. If a random variable X has Negative Binomial distribution with parameters p and m, its probability mass function is:

$P(X=n) = {n-1 \choose m-1} p^m (1-p)^{n-m} \mbox{, for } n \ge m$.

### Example

A travelling salesman goes home if he has sold 3 encyclopedias that day. Some days he sells them quickly. Other days he's out till late in the evening. If on the average he sells an encyclopedia at one out of ten houses he approaches, what is the probability of returning home after having visited only 10 houses?

The number of trials X is Negative Binomial distributed with parameters p=0.1 and m=3, hence:

$P(X=10) = {9 \choose 2} 0.1^3 0.9^7 = 0.017$.

# Continuous Distributions

A continuous statistic is a random variable that does not have any points at which there is any distinct probability that the variable will be the corresponding number.

## Cumulative Distribution Function

A continuous random variable, like a discrete random variable, has a cumulative distribution function. Like the one for a discrete random variable, it also increases towards 1. Depending on the random variable, it may reach one at a finite number, or it may not. The cdf is represented by a capital F.

## Probability Distribution Function

Unlike a discrete random variable, a continuous random variable has a probability density function instead of a probability mass function. The difference is that the former must integrate to 1, while the latter must have a total value of 1. The two are very similar, otherwise. The pdf is represented by a lowercase f.

## Special Values

The expected value for a continuous variable is defined as $\int_{-\infty}^{\infty} xf(x)\, dx$

The expected value of any function of a continuous variable g(x) is defined as $\int_{-\infty}^{\infty} g(x)f(x)\, dx$

The mean of a continuous or discrete distribution is defined as E[X]

The variance of a continuous or discrete distribution is defined as E[(X-E[X]2)]

Expectations can also be derived by producing the Moment Generating Function for the distribution in question. This is done by finding the expected value E[etX]. Once the Moment Generating Function has been created, each derivative of the function gives a different piece of information about the distribution function.

d1x / d1y = mean
d2x / d2y = variance
d3x / d3y = skewness
d4x / d4y = kurtosis

# Uniform Distribution

The uniform distribution, as its name suggests, is a distribution with probability densities that are the same at each point in an interval. In casual terms, the uniform distribution shapes like a rectangle.

Mathematically speaking, the probability density function of the uniform distribution is defined as

$f\left(x\right)= \begin{cases} {1 \over {b-a}}\ \forall\ real\ x\ \in [a,b] \end{cases}$

And the cumulative distribution function is:

$F\left(x\right)= \begin{cases} 0, & \mbox{if } x \le a \ {{x-a} \over {b-a}}, & \mbox{if } a < x < b\ 1, & \mbox{if } x \ge b \end{cases}$

# Normal Distribution

The Normal Probability Distribution is one of the most useful and more important distributions in statistics. It is a continuous variable distribution. Although the mathematics of this distribution can be quite off putting for students of a first course in statistics it can nevertheless be usefully applied with out over complication.

The Normal distribution is used frequently in statistics for many reasons:

1) The Normal distribution has many convenient mathematical properties.

2) Many natural phenomena have distributions which when studied have been shown to be close to that of the Normal Distribution.

3) The Central Limit Theorem shows that the Normal Distribution is a suitable model for large samples regardless of the actual distribution.

## Mathematical Characteristics of the Normal Distribution

A continuous random variable , X, is normally distributed with a probability density function :

$\frac1{\sigma\sqrt{2\pi}}\; \exp\left(-\frac{\left(x-\mu\right)^2}{2\sigma^2} \right) \!$

# F Distribution

Named after Sir Ronald Fisher, who developed the F distribution for use in determining ANOVA critical values. The cutoff values in an F table are found using three variables- ANOVA numerator degrees of freedom, ANOVA denominator degrees of freedom, and significance level.

ANOVA is an abbreviation of analysis of variance. It compares the size of the variance between two different samples. This is done by dividing the larger variance over the smaller variance. The formula of the F statistic is:

$F(r_1, r_2) = \frac{\chi_{r1} ^2 /r_1}{\chi_{r2} ^2 /r_2}$

where $\chi_{r1}^2$ and $\chi_{r2}^2$ are the chi-square statistics of sample one and two respectively, and r1and r2 are their degrees of freedom, i.e. the number of observations.

One example could be if you want to compare apples that look alike but are from different trees and have different sizes. You want to investigate whether they have the same variance of the weight on average.

There are three apples from the first tree that weigh 110, 121 and 143 grams respectively, and four from the other which weigh 88, 93, 105 and 124 grams respectively. The mean and variance of the first sample are 124.67 and 16.80 respectively, and of the second sample 102.50 and 16.01. The chi-square statistic of the first sample is

$\frac{110-124.67}{16.80^2} + \frac{121-124.67}{16.80^2} + \frac{143-124.67}{16.80^2} = 2.00$,

and for the second sample

$\frac{88-102.50}{16.01^2} + \frac{93-102.50}{16.01^2} + \frac{105-102.50}{16.01^2} + \frac{124-102.50}{16.01^2} = 3.00$.

The F statistic is now F = $\frac{3/4}{2/3} = 1.125$. The Chi-square statistic divided by degrees of freedom appears on the nominator for the second sample because it was larger than that of the first sample.

The critical value of the F distribution for 4 degrees of freedom. in the nominator and 3 degrees of freedom in the denominator, i.e. F(f1=4, f2=3) is 9.12 at a 5% level of confidence. Since the test statistic 1.125 is smaller than the critical value, we cannot reject the null hypothesis that they have the same variance. The conclusion is that they have the same variance.

# Testing Statistical Hypothesis

There are many different tests for the many different kinds of data. A way to get started is to understand what kind of data you have. Are the variables quantitative or qualitative? Certain tests are for certain types of data depending on the size, distribution or scale. Also, it is important to understand how samples of data can differ. The 3 primary characteristics of quantitative data are: central tendency, spread, and shape.

When most people "test" quantitative data, they tend to do tests for central tendency. Why? Well, let's say you had 2 sets of data and you wanted to see if they were different from each other. One way to test this would be to test to see if their central tendency (their means for example) differ.

Imagine two symmetric, bell shaped curves with a vertical line drawn directly in the middle of each. If one sample was a lot different than another (a lot higher in values,etc.) then the means would be different typically. So when testing to see if two samples are different, usually two means are compared.

Two medians (another measure of central tendency) can be compared also. Or perhaps one wishes to test two samples to see if they have the same spread or variation. Because statistics of central tendency, spread, etc. follow different distributions - different testing procedures must be followed and utilized.

In the end, most folks summarize the result of a hypothesis test into one particular value - the p-value. If the p-value is smaller than the level of significance (usually α = 5%, but even lower in other fields of science i.e. Medicine) then the zero-hypothesis rejected and the alternative hypothesis accepted. The p-value is actually the probability of making a statistical error. If the p-value is higher than the level of significance you accept the zero-hypothesis and reject the alternative hypothesis, however that does not necessarily mean that the zero-hypothesis is correct.

# Purpose of Statistical Tests

## Purpose of Statistical Tests

In general, the purpose of statistical tests is to determine whether some hypothesis is extremely unlikely given observed data. Note that there are two philosophical approaches to such tests. The first approach, significance testing (due to Fisher), is aimed at quantifying the evidence against a particular hypothesis being true. The second approach, hypothesis testing (due to Neyman and Pearson), is aimed at making a simple decision as to whether to reject or retain a hypothesis. The difference is important in that the evaluation of evidence takes place in context and will lead to opinions that can be revised when new evidence becomes available. However, once a decision has been taken, it is final and cannot be changed. This important difference is frequently overlooked and statisticians often treat the terms "significance test" and "hypothesis test" as though they are interchangeable. They are not!

A data analyst frequently wants to know whether there is a difference between two sets of data, and whether that difference is likely to occur due to random fluctuations, or is instead unusual enough that random fluctuations rarely cause such differences.

In particular, frequently we wish to know something about the average (or mean), or about the variability (as measured by variance or standard deviation).

Statistical tests are carried out by first making some assumption, called the Null Hypothesis, and then determining whether the data observed is unlikely to occur given that assumption. If the probability of seeing the observed data is small enough under the assumed Null Hypothesis, then the Null Hypothesis is rejected.

A simple example might help. We wish to determine if men and women are the same height on average. We select and measure 20 women and 20 men. We assume the Null Hypothesis that there is no difference between the average value of heights for men vs. women. We can then test using the t test to determine whether our sample of 40 heights would be unlikely to occur given this assumption. The basic idea is to assume heights are normally distributed, and to assume that the means and standard deviations are the same for women and for men. Then we calculate the average of our 20 men, and of our 20 women, we also calculate the sample standard deviation for each. Then using the t-test of two means with 40-2 = 38 degrees of freedom we can determine whether the difference in heights between the sample of men and the sample of women is sufficiently large to make it unlikely that they both came from the same normal population.

# Different Types of Tests

A statistical test is always about one or more parameters of the concerned population (distribution). The appropiate test depends on the type of null and alternative hypothesis about this (these) parameter(s) and the available information from the sample.

## Example

It is conjectured that British children gain more weight lately. Hence the population mean μ of the weight X of children of let's say 12 years of age is the parameter at stake. In the recent past the mean weight of this group of children turned out to be 45 kg. Hence the null hypothesis (of no change) is:

$\,H_0: \mu = 45$.

As we suspect a gain in weight, the alternative hypothesis is:

$\,H_1: \mu > 45$.

A random sample of 100 children shows an average weight of 47 kg with a standard deviation of 8 kg.

Because it is reasonable to assume that the weights are normally distributed, the appropriate test will be a t-test, with test statistic:

$T = \frac{\bar{X} - 45}{S}\sqrt{100}$.

Under the null hypothesis T will be Student distributed with 99 degrees of freedom, which means approximately standard normally distributed.

The null hypothesis will be rejected for large values of T. For this sample the value t of T is:

$t = \frac{47 - 45}{8}\sqrt{100} = 2.5$.

Is this a large value? That depends partly on our demands. The so called p-value of the observed value t is:

$p=P(T\ge t; H_0)= P(T\ge 2.5; H_0) \approx P(Z\ge 2.5) <0.01$,

in which Z stands for a standard normally distributed random variable.

If we are not too critical this is small enough, so reason to reject the null hypothesis and to assume our conjecture to be true.

Now suppose we have lost the individual data, but still know that the maximum weight in the sample was 68 kg. It is not possible then to use the t-test, and instead we have to use a test based on the statistic max(X).

It might also be the case that our assumption on the distribution of the weight is questionable. To avoid discussion we may use a distribution free test instead of a t-test.

A statistical test begins with a hypothesis; the form of that hypothesis determines the type(s) of test(s) that can be used. In some cases, only one is appropriate; in others, one may have some choice.

For example: if the hypothesis concerns the value of a single population mean (μ), then a one sample test for mean is indicated. Whether the z-test or t-test should be used depends on other factors (each test has its own requirements).

A complete listing of the conditions under which each type of test is indicated is probably beyond the scope of this work; refer to the sections for the various types of tests for more information about the indications and requirements for each test.

# z Test for a Single Mean

The Null Hypothesis should be an assumption concerning the value of the population mean. The data should consist of a single sample of quantitative data from the population.

## Requirements

The sample should be drawn from a population from which the Standard Deviation (or Variance) is known. Also, the measured variable (typically listed as x—$\bar x$ is the sample statistic) should have a Normal Distribution.

Note that if the distribution of the variable in the population is non-normal (or unknown), the z-test can still be used for approximate results, provided the sample size is sufficiently large. Historically, sample sizes of at least 30 have been considered sufficiently large; reality is (of course) much more complicated, but this rule of thumb is still in use in many textbooks.

If the population Standard Deviation is unknown, then a z-test is typically not appropriate. However, when the sample size is large, the sample standard deviation can be used as an estimate of the population standard deviation, and a z-test can provide approximate results.

## Definitions of Terms

μ; = Population Mean
σ < sub > x < / sub > = Population Standard Deviation
$\bar x$ = Sample Mean
$\sigma\bar x$ = Sample Standard Deviation
N = Sample Population

## Procedure

• The Null Hypothesis:

This is a statement of no change or no effect; often, we are looking for evidence that this statement is no longer true.

H0 : μ = μ0
• The Alternate Hypothesis:

This is a statement of inequality; we are looking for evidence that this statement is true.

H1 : μ < μ0 or
H1 : μ > μ0 or
H1 : μ ≠ μ0
• The Test Statistic:
$z=\frac{\bar x -\mu _0}{\sigma / \sqrt{n}}$
• The Significance (p-value)

Calculate the probability of observing a value of z (from a Standard Normal Distribution) using the Alternate Hypothesis to indicate the direction in which the area under the Probability Density Function is to be calculated. This is the Attained Significance, or p-value.

Note that some (older) methods first chose a Level Of Significance, which was then translated into a value of z. This made more sense (and was easier!) in the days before computers and graphics calculators.

• Decision

The Attained Significance represents the probability of obtaining a test statistic as extreme, or more extreme, than ours—if the null hypothesis is true.

If the Attained Significance (p-value) is sufficiently low, then this indicates that our test statistic is unusual (rare)—we usually take this as evidence that the null hypothesis is in error. In this case, we reject the null hypothesis.

If the p-value is large, then this indicates that the test statistic is usual (common)—we take this as a lack of evidence against the null hypothesis. In this case, we fail to reject the null hypothesis.

It is common to use 5% as the dividing line between the common and the unusual; again, reality is more complicated. Sometimes a lower level of uncertainty must be chosen should the consequences of error results in a decision that can injure or kill people or do great economic harm. We would more likely tolerate a drug that kills 5% of patients with a terminal cancer but cures 95% of all patients, but we would hardly tolerate a cosmetic that disfigures 5% of those who use it.

## Worked Examples

### Are The Kids Above Average?

Scores on a certain test of mathematical aptitude have mean μ = 50 and standard deviation σ = 10. An amateur researcher believes that the students in his area are brighter than average, and wants to test his theory.

The researcher has obtained a random sample of 45 scores for students in his area. The mean score for this sample is 52.

Does the researcher have evidence to support his belief?

The null hypothesis is that there is no difference, and that the students in his area are no different than those in the general population; thus,

H0 : μ = 50

(where μ represents the mean score for students in his area)

He is looking for evidence that the students in his area are above average; thus, the alternate hypothesis is

H1 : μ > 50

Since the hypothesis concerns a single population mean, a z-test is indicated. The sample size is fairly large (greater than 30), and the standard deviation is known, so a z-test is appropriate.

$z=\frac{\bar x -\mu _0}{\sigma / \sqrt{n}} =\frac{52-50}{10/ \sqrt{45}}=1.3416$

We now find the area under the Normal Distribution to the right of z = 1.3416 (to the right, since the alternate hypothesis is to the right). This can be done with a table of values, or software—I get a value of 0.0899.

If the null hypothesis is true (and these students are no better than the general population), then the probability of obtaining a sample mean of 52 or higher is 8.99%. This occurs fairly frequently (using the 5% rule), so it does not seem unusual. I fail to reject the null hypothesis (at the 5% level).

It appears that the evidence does not support the researcher's belief.

### Is The Machine Working Correctly?

Sue is in charge of Quality Control at a bottling facility. Currently, she is checking the operation of a machine that is supposed to deliver 355 mL of liquid into an aluminum can. If the machine delivers too little, then the local Regulatory Agency may fine the company. If the machine delivers too much, then the company may lose money. For these reasons, Sue is looking for any evidence that the amount delivered by the machine is different from 355 mL.

During her investigation, Sue obtains a random sample of 10 cans, and measures the following volumes:

355.02 355.47 353.01 355.93 356.66 355.98 353.74 354.96 353.81 355.79

The machine's specifications claim that the amount of liquid delivered varies according to a normal distribution, with mean μ = 355 mL and standard deviation σ = 0.05 mL.

Do the data suggest that the machine is operating correctly?

The null hypothesis is that the machine is operating according to its specifications; thus

H0 : μ = 355

(where μ is the mean volume delivered by the machine)

Sue is looking for evidence of any difference; thus, the alternate hypothesis is

H1 : μ ≠ 355

Since the hypothesis concerns a single population mean, a z-test is indicated. The population follows a normal distribution, and the standard deviation is known, so a z-test is appropriate.

In order to calculate the test statistic (z), we must first find the sample mean from the data. Use a calculator or computer to find that $\bar x = 355.037$.

$z=\frac{\bar x -\mu _0}{\sigma / \sqrt{n}} =\frac{355.037-355}{0.05/ \sqrt{10}}=2.34$

The calculation of the p-value will be a little different. If we only find the area under the normal curve above z = 2.34, then we have found the probability of obtaining a sample mean of 355.037 or higher—what about the probability of obtaining a low value?

In the case that the alternate hypothesis uses ≠, the p-value is found by doubling the tail area—in this case, we double the area above z = 2.34.

The area above z = 2.34 is 0.0096; thus, the p-value for this test is 0.0192.

If the machine is delivering 355 mL, then the probability of obtaining a sample mean this far (0.037 mL) or farther from 355 mL is 0.0096, or 0.96%. This is pretty rare; I'll reject the null hypothesis.

It appears that the machine is not working correctly.

N.B.: since the alternate hypothesis is ≠, we cannot conclude that the machine is delivering more than 355 mL—we can only say that the amount is different from 355 mL.

# z Test for Two Means

## Indications

The Null Hypothesis should be an assumption about the difference in the population means for two populations (note that the same quantitative variable must have been measured in each population). The data should consist of two samples of quantitative data (one from each population). The samples must be obtained independently from each other.

## Requirements

The samples must be drawn from populations which have known Standard Deviations (or Variances). Also, the measured variable in each population (generically denoted x1 and x2) should have a Normal Distribution.

Note that if the distributions of the variables in the populations are non-normal (or unknown), the two-sample z-test can still be used for approximate results, provided the combined sample size (sum of sample sizes) is sufficiently large. Historically, a combined sample size of at least 30 has been considered sufficiently large; reality is (of course) much more complicated, but this rule of thumb is still in use in many textbooks.

## Procedure

• The Null Hypothesis:
H0 : μ1 - μ2 = δ

in which δ is the supposed difference in the expected values under the null hypothesis.

• The Alternate Hypothesis:
H0 : μ1 - μ2 < δ
H0 : μ1 - μ2 > δ
H0 : μ1 - μ2 ≠ δ

For more information about the Null and Alternate Hypotheses, see the page on the z test for a single mean.

• The Test Statistic:
$z=\frac{(\bar{x}_1 - \bar{x}_2) - \delta}{\sqrt{\frac{\sigma _1^2}{n_1}+\frac{\sigma _2^2}{n_2}}}$

Usually, the null hypothesis is that the population means are equal; in this case, the formula reduces to

$z= \frac{\bar{x}_1 - \bar{x}_2}{\sqrt{\frac{\sigma _1^2}{n_1}+\frac{\sigma _2^2}{n_2}}}$

In the past, the calculations were simpler if the Variances (and thus the Standard Deviations) of the two populations could be assumed equal. This process is called Pooling, and many textbooks still use it, though it is falling out of practice (since computers and calculators have all but removed any computational problems).

$\frac{\bar{x}_1 - \bar{x}_2} {\sigma \sqrt{\frac{1}{n_1} + \frac{1}{n_2}}}$
• The Significance (p-value)

Calculate the probability of observing a value of z (from a Standard Normal Distribution) using the Alternate Hypothesis to indicate the direction in which the area under the Probability Density Function is to be calculated. This is the Attained Significance, or p-value.

Note that some (older) methods first chose a Level Of Significance, which was then translated into a value of z. This made more sense (and was easier!) in the days before computers and graphics calculators.

• Decision

The Attained Significance represents the probability of obtaining a test statistic as extreme, or more extreme, than ours—if the null hypothesis is true.

If the Attained Significance (p-value) is sufficiently low, then this indicates that our test statistic is unusual (rare)—we usually take this as evidence that the null hypothesis is in error. In this case, we reject the null hypothesis.

If the p-value is large, then this indicates that the test statistic is usual (common)—we take this as a lack of evidence against the null hypothesis. In this case, we fail to reject the null hypothesis.

It is common to use 5% as the dividing line between the common and the unusual; again, reality is more complicated.

## Worked Examples

### Do Professors Make More Money at Larger Universities?

Universities and colleges in the United States of America are categorized by the highest degree offered. Type IIA institutions offer a Master's Degree, and type IIB institutions offer a Baccalaureate degree. A professor, looking for a new position, wonders if the salary difference between type IIA and IIB institutions is really significant.

He finds that a random sample of 200 IIA institutions has a mean salary (for full professors) of $54,218.00, with standard deviation$8,450. A random sample of 200 IIB institutions has a mean salary (for full professors) of $46,550.00, with standard deviation$9,500 (assume that the sample standard deviations are in fact the population standard deviations).

Do these data indicate a significantly higher salary at IIA institutions?

The null hypothesis is that there is no difference; thus

H0 : μA = μB

(where μA is the true mean full professor salary at IIA institutions, and μB is the mean at IIB institutions)

He is looking for evidence that IIA institutions have a higher mean salary; thus the alternate hypothesis is

H1 : μA > μB

Since the hypotheses concern means from independent samples (we'll assume that these are independent samples), a two sample test is indicated. The samples are large, and the standard deviations are known (assumed?), so a two sample z-test is appropriate.

$z=\frac{\mu _A -\mu _B}{\sqrt{\frac{\sigma _A ^2}{n _A}+\frac{\sigma _B ^2}{n _B}}}= \frac{54218-46550}{\sqrt{\frac{8450 ^2}{200}+\frac{9500 ^2}{200}}}= 8.5292$

Now we find the area to the right of z = 8.5292 in the Standard Normal Distribution. This can be done with a table of values or software—I get 0.

If the null hypothesis is true, and there is no difference in the salaries between the two types of institutions, then the probability of obtaining samples where the mean for IIA institutions is at least \$7,668 higher than the mean for IIB institutions is essentially zero. This occurs far too rarely to attribute to chance variation; it seems quite unusual. I reject the null hypothesis (at any reasonable level of significance!).

It appears that IIA schools have a significantly higher salary than IIB schools.

# t Test for a single mean

The t- test is the most powerful parametric test for calculating the significance of a small sample mean.

A one sample t-test has the following null hypothesis:

$H_0: \quad \mu=c$

where the Greek letter μ (mu) represents the population mean and c represents its assumed (hypothesized) value. In statistics it is usual to employ Greek letters for population parameters and Roman letters for sample statistics. The t-test is the small sample analog of the z test which is suitable for large samples. A small sample is generally regarded as one of size n<30.

A t-test is necessary for small samples because their distributions are not normal. If the sample is large (n>=30) then statistical theory says that the sample mean is normally distributed and a z test for a single mean can be used. This is a result of a famous statistical theorem, the Central limit theorem.

A t-test, however, can still be applied to larger samples and as the sample size n grows larger and larger, the results of a t-test and z-test become closer and closer. In the limit, with infinite degrees of freedom, the results of t and z tests become identical.

In order to perform a t-test, one first has to calculate the "degrees of freedom." This quantity takes into account the sample size and the number of parameters that are being estimated. Here, the population parameter, mu is being estimated by the sample statistic x-bar, the mean of the sample data. For a t-test the degrees of freedom of the single mean is n-1. This is because only one population parameter (the population mean)is being estimated by a sample statistic (the sample mean).

degrees of freedom (df)=n-1


For example, for a sample size n=15, the df=14.

### Example

A college professor wants to compare her students' scores with the national average. She chooses an SRS of 20 students, who score an average of 50.2 on a standardized test. Their scores have a standard deviation of 2.5. The national average on the test is a 60. She wants to know if her students scored significantly lower than the national average.

Significance tests follow a procedure in several steps.

#### Step 1

First, state the problem in terms of a distribution and identify the parameters of interest. Mention the sample. We will assume that the scores (X) of the students in the professor's class are approximately normally distributed with unknown parameters μ and σ

#### Step 2

State the hypotheses in symbols and words.

$H_O: \quad \mu=60$

The null hypothesis is that her students scored on par with the national average.

$H_A: \quad \mu<60$

The alternative hypothesis is that her students scored lower than the national average.

#### Step 3

Secondly, identify the test to be used. Since we have an SRS of small size and do not know the standard deviation of the population, we will use a one-sample t-test.

The formula for the t-statistic T for a one-sample test is as follows:

$T = \frac{\overline{X} - 60}{S/\sqrt{20}}$

where $\overline{X}$ is the sample mean and S is the sample standard deviation.

A quite common mistake is to say that the formula for the t-test statistic is:

$T = \frac{\overline{x} - \mu}{s/\sqrt{n}}$

This is not a statistic, because μ is unknown, which is the crucial point in such a problem. Most people even don't notice it. Another problem with this formula is the use of x and s. They are to be considered the sample statistics and not their values.

The right general formula is:

$T = \frac{\overline{X} - c}{S/\sqrt{n}}$

in which c is the hypothetical value for μ specified by the null hypothesis.

(The standard deviation of the sample divided by the square root of the sample size is known as the "standard error" of the sample.)

#### Step 4

State the distribution of the test statistic under the null hypothesis. Under H0 the statistic T will follow a Student's distribution with 19 degrees of freedom: $T \sim \tau\cdot(20-1)$.

#### Step 5

Compute the observed value t of the test statistic T, by entering the values, as follows:

$t = \frac{\overline{x} - 60}{s/\sqrt{20}} = \frac{4.95 - 5.00}{0.45/\sqrt{8}} = \frac{-9.8}{2.5/4.47} = \frac{-9.8}{0.559} = -17.5$

#### Step 6

Determine the so-called p-value of the value t of the test statistic T. We will reject the null hypothesis for too small values of T, so we compute the left p-value:

p-value $= P(T \leq t ;H_0) = P(T(19) \leq -17.5) \approx 0$

The Student's distribution gives T(19) = 1.729 at probabilities 0.95 and degrees of freedom 19. The p-value is approximated at 1.777e-13.

#### Step 7

Lastly, interpret the results in the context of the problem. The p-value indicates that the results almost certainly did not happen by chance and we have sufficient evidence to reject the null hypothesis. The professor's students did score significantly lower than the national average.

# t Test for Two Means

In both the one- and two-tailed versions of the small two-sample t-test, we assume that the means of the two populations are equal. To use a t-test for small (independent) samples, the following conditions must be met:

1. The samples must be selected randomly.
2. The samples must be independent.
3. Each population must have a normal distribution.

A small two sample t-test is used to test the difference between two population means m1 and m2 when the sample size for at least one population is less than 30.The standardized test statistic is:

# One-Way ANOVA F Test

The one-way ANOVA F-test is used to identify if there are between subject effects. For instance, to investigate the effect of a certain new drug on the number of white blood cells, in an experiment the drug is given to three different groups, one of healthy people, one with people with a light form of the considered disease and one with a severe form of the disease. Generally the analysis of variance identifies whether there is a significant difference in effect of the drug on the number of white blood cells between the groups. Significant refers to the fact that there will always be difference between the groups and also within the groups, but the purpose is to investigate whether the difference between the groups are large compared to the differences within the groups. To set up such an experiment three assumptions must be validated before calculating an F statistic: independent samples, homogeneity of variance, and normality. The first assumption suggests that there is no relation between the measurements for different subjects. Homogeneity of variance refers to equal variances among the different groups in the experiment (e.g., drug vs. placebo). Furthermore, the assumption of normality suggests that the distribution of each of these groups should be approximately normally distributed.

## Model

The situation is modelled in the following way. The measurement of the j-th test person in group i is indicated by:

$X_{ij}=\mu+\alpha_i+U_{ij}\,$.

This reads: the outcome of the measurement for j in group i is due to a general effect indicated by $\mu\,$, an effect due to the group, $\alpha_i\,$ and an individual contribution $U_{ij}\,$.

The individual, or random, contributions $U_{ij}\,$, often referred to as disturbances, are considered to be independently, normally distributed, all with expected value 0 and standard deviation σ.

To make the model unambiguous the group effects are restrained by the condition:

$\sum_i\alpha_i=0\,$.

Now. a notational note: it is common practice to indicate averages over one or more indices by writing a dot in the place of the index or indices. So for instance

$X_{i.} = \frac{1}{N}\sum^N_{j=1} X_{ij}$

The analysis of variance now divides the total "variance" in the form of the total "sum of squares" in two parts, one due to the variation within the groups and one due to the variation between the groups:

$SST=\sum_{ij}(X_{ij}-X{..})^2=\sum_{ij}(X_{ij}-X_{i.}+X_{i.}-X{..})^2= \sum_{ij}(X_{ij}-X_{i.})^2+\sum_{ij}(X_{i.}-X{..})^2\,$.

We see the term sum of squares of error:

$SSE=\sum_{ij}(X_{ij}-X_{i.})^2\,$

of the total squared differences of the individual measurements from their group averages, as an indication of the variation within the groups, and the term sum of square of the factor

$SSA=\sum_{ij}(X_{i.}-X{..})^2\,$

of the total squared differences of the group means from the overall mean, as an indication of the variation between the groups.

Under the null hypothesis of no effect:

$H_0: \forall_i\ \alpha_i=0$

we find:

$SSE/\sigma^2\,$ is chi-square distributed with a(m-1) degrees of freedom, and
$SSA/\sigma^2\,$ is chi-square distributed with a-1 degrees of freedom,

where a is the number of groups and m is the number of persons in each group.

Hence the quotient of the so-called mean sum of squares:

$MSA=\frac{SSA}{a-1}$

and

$MSE=\frac{SSE}{a(m-1)}$

may be used as a test statistic

$F=\frac{MSA}{MSE}$

which under the null hypothesis is F-distributed with a − 1 degrees of freedom in the nominator and a(m − 1) in the denominator, because the unknown parameter σ does not play a role since it is cancelled out in the quotient.

# Testing whether Proportion A Is Greater than Proportion B in Microsoft Excel

A running example from the 2004 American Presidential Race follows. It should be clear that the choice of poll and who is leading is irrelevant to the presentation of the concepts. According to an October 2nd Poll by Newsweek (link), 47% of 1,013 registered voters would vote for John Kerry/John Edwards if the election were held today. 45% would vote for George Bush/Dick Cheney, and 2% would vote for Ralph Nader/Peter Camejo.

• Open a new Blank Workbook in the program Microsoft Excel.
• Enter Kerry's reported percentage p in cell A1 (0.47).
• Enter Bush's reported percentage q in cell B1 (0.45).
• Enter the number of respondents N in cell C1 (1013). This can be found in most responsible reports on polls.
• In cell A2, copy and paste the next line of text in its entirety and press Enter. This is the Microsoft Excel expression of the standard error of the difference as shown above.
=sqrt(A1*(1-A1)/C1+B1*(1-B1)/C1+2*A1*B1/C1)
• In cell A3, copy and paste the next line of text in its entirety and press Enter. This is the Microsoft Excel expression of the probability that Kerry is leading based on the normal distribution given the logic here.
=normdist((A1-B1),0,A2,1)
• Don't forget that the percentages will be in decimal form. The percentage will be 0.5, or 50% if A1 and B1 are the same, of course.

The above text might be enough to do the necessary calculation, it doesn't contribute to the understanding of the statistical test involved. Much too often people think statistics is a matter of calculation with complex formulas.

So here is the problem: Let p be the population fraction of the registered voters who vote for Kerry and q likewise for Bush. In a poll n = 1013 respondents are asked to state their choice. A number of K respondents says to choose Kerry, a number B says to vote for Bush. K and B are random variables. The observed values for K and B are resp. k and b (numbers). So k/n is an estimate of p and b/n an estimate of q. The random variables K and B follow a trinomial distribution with parameters n, p, q and 1-p-q. Will Kerry be ahead of Bush? That is to say: wiil p > q? To investigate this we perform a statistical test, with null hypothesis:

$\, H_0: p = q$

against the alternative

$\, H_1: p > q$.

What is an appropriate test statistic T? We take:

$\, T=K-B$.

(In the above calculation $T=\frac Kn - \frac Bn = \frac{K-B}n$ is taken, which leads to the same calculation.)

We have to state the distribution of T under the null hypothesis. We may assume T is approximately normally distributed.

It is quite obvious that its expectation under H0 is:

$\, E_0T = 0$.

Its variance under H0 is not as obvious.

$\, var_0(T) = var(K-B) = var(K) + var(B) - 2cov(K,B) = np(1-p) + nq(1-q) + 2npq$.

We approximate the variance by using the sample fractions instead of the population fractions:

$var_0(T) \approx 1013\times 0.47(1-0,46) + 1013\times 0.45(1-0.45) + 2\times 1013\times 0,47\times0.45 \approx 931$.

The standard deviation s will approximately be:

$\, s = \sqrt{var_0(T)} \approx \sqrt{931} = 30.5$.

In the sample we have found a value t = k - b = (0.47-0.45)1013 = 20.26 for T. We will reject the null hypothesis in favour of the alternative for large values of T. So the question is: is 20.26 to be considered a large value for T? The criterion will be the so called p-value of this outcome:

$\, p-value = P(T\ge t; H_0) = P(T\ge 20.26; H_0) = P(Z\ge \frac{20.26}{30.5}) = 1-\Phi(0.67) = 0.25$.

This is a very large p-value, so there is no reason whatsoever to reject the null hypothesis.

# Chi-Squared Tests

## General idea

Assume you have observed absolute frequencies oi and expected absolute frequencies ei under the Null hypothesis of your test then it holds

$V = \sum_i \frac{(o_i-e_i)^2}{e_i} \approx \chi^2_f .$

i might denote a simple index running from 1,...,I or even a multiindex (i1,...,ip) running from (1,...,1) to (I1,...,Ip).

The test statistics V is approximately χ2 distributed, if

1. for all absolute expected frequencies ei holds $e_i \geq 1$ and
2. for at least 80% of the absolute expected frequencies ei holds $e_i \geq 5$.

Note: In different books you might find different approximation conditions, please feel free to add further ones.

The degrees of freedom can be computed by the numbers of absolute observed frequencies which can be chosen freely. We know that the sum of absolute expected frequencies is

 ∑ oi = n i

which means that the maximum number of degrees of freedom is I − 1. We might have to subtract from the number of degrees of freedom the number of parameters we need to estimate from the sample, since this implies further relationships between the observed frequencies.

## Derivation of the distribution of the test statistic

Following Boero, Smith and Wallis (2002) we need knowledge about multivariate statistics to understand the derivation.

The random variable O describing the absolute observed frequencies (o1,...,ok) in a sample has a multinomial distribution $O \sim M(n;p_1,...,p_k)$ with n the number of observations in the sample, pi the unknown true probabilities. With certain approximation conditions (central limit theorem) it holds that

$O \sim M(n; p_1,...,p_k) \approx N_k(\mu;\Sigma)$

with Nk the multivariate k dimensional normal distribution, μ = (np1,...,npk) and

$\Sigma = (\sigma_{ij})_{i,j=1,...,k} = \begin{cases} -np_ip_j, & \mbox{if } i\neq j \\ np_i(1-p_i) & \mbox{otherwise} \end{cases}$.

The covariance matrix Σ has only rank k − 1, since p1 + ... + pk = 1.

If we considered the generalized inverse Σ then it holds that

$(O-\mu)^T \Sigma^- (O-\mu) = \sum_i \frac{(o_i-e_i)^2}{e_i} \sim \chi^2_{k-1}$

distributed (for a proof see Pringle and Rayner, 1971).

Since the multinomial distribution is approximately multivariate normal distributed, the term is

$\sum_i \frac{(o_i-e_i)^2}{e_i} \approx \chi^2_{k-1}$

distributed. If further relations between the observed probabilities are there then the rank of Σ will decrease further.

A common situation is that parameters on which the expected probabilities depend needs to be estimated from the observed data. As said above, usually is stated that the degrees of freedom for the chi square distribution is k − 1 − r with r the number of estimated parameters. In case of parameter estimation with the maximum-likelihood method this is only true if the estimator is efficient (Chernoff and Lehmann, 1954). In general it holds that degrees of freedom are somewhere between k − 1 − r and k − 1.

## Examples

The most famous examples will be handled in detail at further sections: χ2 test for independence, χ2 test for homogeneity and χ2 test for distributions.

The χ2 test can be used to generate "quick and dirty" test, e.g.

H0: The random variable X is symmetrically distributed versus

H1: the random variable X is not symmetrically distributed.

We know that in case of a symmetrical distribution the arithmetic mean $\bar{x}$ and median should be nearly the same. So a simple way to test this hypothesis would be to count how many observations are less than the mean (n )and how many observations are larger than the arithmetic mean (n + ). If mean and median are the same than 50% of the observation should smaller than the mean and 50% should be larger than the mean. It holds

$V = \frac{(n_- - n/2)^2}{n/2} + \frac{(n_+ - n/2)^2}{n/2} \approx \chi^2_1$.

# Distributions Problems

A normal distribution has μ = 100 and σ = 15. What percent of the distribution is greater than 120?

# Numerical Methods

Often the solution of statistical problems and/or methods involve the use of tools from numerical mathematics. An example might be Maximum-Likelihood estimation of $\widehat{\Theta}$which involves the maximization of the Likelihood function L:

$\widehat{\Theta} = \max_\theta\,\, L(\theta | x_1, ..., x_n)$.

The maximization here requires the use of optimization routines. Other numerical methods and their application in statistics are described in this section.

Contents of this section:

• Basic Linear Algebra and Gram-Schmidt Orthogonalization

This section is dedicated to the Gram-Schmidt Orthogonalization which occurs frequently in the solution of statistical problems. Additionally some results of algebra theory which are necessary to understand the Gram-Schmidt Orthogonalization are provided. The Gram-Schmidt Orthogonalization is an algorithm which generates from a set of linear dependent vectors a new set of linear independent vectors which span the same space. Computation based on linear independent vectors is simpler than computation based on linear dependent vectors.

• Unconstrained Optimization

Numerical Optimization occurs in all kind of problem - a prominent example being the Maximum-Likelihood estimation as described above. Hence this section describes one important class of optimization algorithms, namely the so-called Gradient Methods. After describing the theory and developing an intuition about the general procedure, three specific algorithms (the Method of Steepest Descent, the Newtonian Method, the class of Variable Metric Methods) are described in more detail. Especially we provide an (graphical) evaluation of the performance of these three algorithms for specific criterion functions (the Himmelblau function and the Rosenbrock function). Furthermore we come back to Maximum-Likelihood estimation and give a concrete example how to tackle this problem with the methods developed in this section.

• Quantile Regression

In OLS, one has the primary goal of determining the conditional mean of random variable Y, given some explanatory variable xi , E[Y | xi]. Quantile Regression goes beyond this and enables us to pose such a question at any quantile of the conditional distribution function. It thereby focuses on the interrelationship between a dependent variable and its explanatory variables for a given quantile.

• Numerical Comparison of Statistical Software

Statistical calculations require an extra accuracy and are open to some errors such as truncation or cancellation error etc. These errors occur due to binary representation and finite precision and may cause inaccurate results. In this work we are going to discuss the accuracy of the statistical software, different tests and methods available for measuring the accuracy and the comparison of different packages.

• Numerics in Excel

The purpose of this paper is to evaluate the accuracy of MS Excel in terms of statistical procedures and to conclude whether the MS Excel should be used for (statistical) scientific purposes or not. The evaluation is made for MS Excel versions 97, 2000, XP and 2003.

• Random Number Generation

# Basic Linear Algebra and Gram-Schmidt Orthogonalization

## Introduction

Basically, all the sections found here can be also found in a linear algebra book. However, the Gram-Schmidt Orthogonalization is used in statistical algorithm and in the solution of statistical problems. Therefore, we briefly jump into the linear algebra theory which is necessary to understand Gram-Schmidt Orthogonalization.

The following subsections also contain examples. It is very important for further understanding that the concepts presented here are not only valid for typical vectors as tuple of real numbers, but also functions that can be considered vectors.

## Fields

### Definition

A set R with two operations + and * on its elements is called a field (or short (R, + , * )), if the following conditions hold:

1. For all $\alpha, \beta \in R$ holds $\alpha+\beta \in R$
2. For all $\alpha, \beta \in R$ holds α + β = β + α (commutativity)
3. For all $\alpha, \beta,\gamma \in R$ holds α + (β + γ) = (α + β) + γ (associativity)
4. It exist a unique element 0, called zero, such that for all $\alpha \in R$ holds α + 0 = α
5. For all $\alpha \in R$ a unique element − α, such that holds α + ( − α) = 0
6. For all $\alpha, \beta \in R$ holds $\alpha*\beta \in R$
7. For all $\alpha, \beta \in R$ holds α * β = β * α (commutativity)
8. For all $\alpha, \beta,\gamma \in R$ holds α * (β * γ) = (α * β) * γ (associativity)
9. It exist a unique element 1, called one, such that for all $\alpha \in R$ holds α * 1 = α
10. For all non-zero $\alpha \in R$ a unique element α − 1, such that holds α * α − 1 = 1
11. For all $\alpha, \beta,\gamma \in R$ holds α * (β + γ) = α * β + α * γ (distributivity)

The elements of R are also called scalars.

### Examples

It can easily be proven that real numbers with the well known addition and multiplication (IR, + , * ) are a field. The same holds for complex numbers with the addition and multiplication. Actually, there are not many more sets with two operations which fulfill all of these conditions.

For statistics, only the real and complex numbers with the addition and multiplication are important.

## Vector spaces

### Definition

A set V with two operations + and * on its elements is called a vector space over R, if the following conditions hold:

1. For all $x, y\in V$ holds $x+y \in V$
2. For all $x, y \in V$ holds x + y = y + x (commutativity)
3. For all $x, y, z \in V$ holds x + (y + z) = (x + y) + z (associativity)
4. It exist a unique element $\mathbb{O}$, called origin, such that for all $x \in V$ holds $x+\mathbb{O} = x$
5. For all $x \in V$ exists a unique element v, such that holds $x+ (-x) = \mathbb{O}$
6. For all $\alpha\in R$ and $x\in V$ holds $\alpha*x \in V$
7. For all $\alpha, \beta \in R$ and $x\in V$ holds α * (β * x) = (α * β) * x (associativity)
8. For all $x\in V$ and $1 \in R$ holds 1 * x = x
9. For all $\alpha\in R$ and for all $x, y\in V$holds α * (x + y) = α * x + α * y (distributivity wrt. vector addition)
10. For all $\alpha, \beta \in R$ and for all $x\in V$holds (α + β) * x = α * x + β * x (distributivity wrt. scalar addition)

Note that we used the same symbols + and * for different operations in R and V. The elements of V are also called vectors.

Examples:

1. The set IRp with the real-valued vectors (x1,...,xp) with elementwise addition x + y = (x1 + y1,...,xp + yp) and the elementwise multiplication α * x = (αx1,...,αxp) is a vector space over IR.
2. The set of polynomials of degree p, P(x) = b0 + b1x + b2x2 + ... + bpxp, with usual addition and multiplication is a vector space over IR.

### Linear combinations

A vector x can be written as a linear combination of vectors x1,...xn, if

$x = \sum_{i=1}^n \alpha_i x_i$

with $\alpha_i \in R$.

Examples:

• (1,2,3) is a linear combination of $(1,0,0),\,(0,1,0), \,(0,0,1)$ since (1,2,3) = 1 * (1,0,0) + 2 * (0,1,0) + 3 * (0,0,1)
• 1 + 2 * x + 3 * x2 is a linear combination of $1+x+x^2,\, x+x^2,\, x^2$ since 1 + 2 * x + 3 * x2 = 1 * (1 + x + x2) + 1 * (x + x2) + 1 * (x2)

### Basis of a vector space

A set of vectors x1,...,xn is called a basis of the vector space V, if

1. for each vector xinV exist scalars $\alpha_1,...,\alpha_n \in R$ such that
 x = ∑ αixi i
and
2. there is no subset of {x1,...,xn} such that 1. is fulfilled.

Note, that a vector space can have several bases.

Examples:

• Each vector $(\alpha_1, \alpha_2, \alpha_3) \in IR^3$ can be written as α1 * (1,0,0) + α2 * (0,1,0) + α3 * (0,0,1). Therefore is {(1,0,0),(0,1,0),(0,0,1)} a basis of IR3.
• Each polynomial of degree p can be written as linear combination of {1,x,x2,...,x p} and therefore forms a basis for this vector space.

Actually, for both examples we would have to prove condition 2., but it is clear that it holds.

### Dimension of a vector space

A dimension of a vector space is the number of vectors which are necessary for a basis. A vector space has infinitely many number of basis, but the dimension is uniquely determined. Note that the vector space may have a dimension of infinity, e.g. consider the space of continuous functions.

Examples:

• The dimension of IR3 is three, the dimension of IRp is p .
• The dimension of the polynomials of degree p is p + 1.

### Scalar products

A mapping $<.,.>: V\times V \rightarrow R$ is called a scalar product if holds for all $x,x_1,x_2,y,y_1,y_2 \in V$ and α12inR

1. < α1x1 + α2x2,y > = α1 < x1,y > + α2 < x2,y >
2. < x1y1 + α2y2 > = α1 < x,y1 > + α2 < x,y2 >
3. $ = \overline{}$ with $\overline{\alpha + \imath \beta} = \alpha - \imath \beta$
4. $ \geq 0$ with $=0 \Leftrightarrow x = \mathbb{O}$

Examples:

• The typical scalar product in IRp is  < x,y > = ∑ xiyi i
.
• $ = \int_a^b f(x)*g(x) dx$ is a scalar product on the vector space of polynomials of degree p.

### Norm

A norm of a vector is a mapping $\|.\|: V \rightarrow R$, if holds

1. $\| x \| \geq 0$ for all $x \in V$ and $\| x \| =0 \Leftrightarrow x=\mathbb{O}$ (positive definiteness)
2. $\| \alpha v \|= \mid \alpha \mid \| x \|$ for all $x\in V$ and all $\alpha\in R$
3. $\| x+y \| \leq \| x \| + \| y \|$ for all $x,y\in V$ (triangle inequality)

Examples:

• The Lq norm of a vector in IRp is defined as $\|x\|_q = \sqrt[q]{\sum_{i=1}^p x_i^q}$.
• Each scalar product generates a norm by $\|x\| = \sqrt{}$, therefore $\|f\| = \sqrt{\int_a^b f^2(x) dx}$ is a norm for the polynomials of degree p.

### Orthogonality

Two vectors x and y are orthogonal to each other if < x,y > = 0. In IRp it holds that the cosine of the angle between two vectors can expressed as

$\cos(\angle(x,y)) = \frac{}{\|x\|\|y\|}$.

If the angle between x and y is ninety degree (orthogonal) then the cosine is zero and it follows that < x,y > = 0.

A set of vectors x1,...,xp is called orthonormal, if

$ = \begin{cases} 0 & \mbox{ if } i\neq j \\ 1 & \mbox{ if } i=j \end{cases}$.

If we consider a basis e1,...,ep of a vector space then we would like to have a orthonormal basis. Why ?

Since we have a basis, each vector x and y can be expressed by x = α1e1 + ... + αpep and y = β1e1 + ... + βpep. Therefore the scalar product of x and y reduces to

 $\$ $= <\alpha_1 e_1 + ... +\alpha_p e_p, \beta_1 e_1 + ... +\beta_p e_p>\$ $= \sum_{i=1}^p \sum_{j=1}^p \alpha_i \beta_j $ $= \sum_{i=1}^p \alpha_i \beta_i $ $= \alpha_1 \beta_1 + ... + \alpha_p \beta_p.\$

Consequently, the computation of a scalar product is reduced to simple multiplication and addition if the coefficients are known. Remember that for our polynomials we would have to solve an integral!

## Gram-Schmidt orthogonalization

### Algorithm

The aim of the Gram-Schmidt orthogonalization is to find for a set of vectors x1,...,xp an equivalent set of orthonormal vectors o1,...,op such that any vector which can be expressed as linear combination of x1,...,xp can also be expressed as linear combination of o1,...,op:

1. Set b1 = x1 and $o_1 = b_1 / \|b_1\|$

2. For each i > 1 set $b_i = x_i - \sum_{j=1}^{i-1} \frac{}{} b_j$ and $o_i = b_i / \|b_i\|$, in each step the vector xi is projected on bj and the result is subtracted from xi.

### Example

Consider the polynomials of degree two in the interval[ − 1,1] with the scalar product $ = \int_{-1}^1 f(x) g(x) dx$ and the norm $\|f\| = \sqrt{}$. We know that f1(x) = 1,f2(x) = x and f3(x) = x2 are a basis for this vector space. Let us now construct an orthonormal basis:

Step 1a: b1(x) = f1(x) = 1

Step 1b: $o_1(x) = \frac{b_1(x)}{\|b_1(x)\|} = \frac{1}{\sqrt{}} = \frac{1}{\sqrt{\int_{-1}^1 1 dx}} = \frac{1}{\sqrt{2}}$

Step 2a: $b_2(x) = f_2(x) - \frac{}{} b_1(x) = x - \frac{\int_{-1}^1 x\ 1 dx}{2} 1 = x - \frac{0}{2} 1 = x$

Step 2b: $o_2(x) = \frac{b_2(x)}{\|b_2(x)\|} = \frac{x}{\sqrt{}} = \frac{x}{\sqrt{\int_{-1}^1 x^2 dx}} = \frac{x}{\sqrt{2/3}} = x\sqrt{3/2}$

Step 3a: $b_3(x) = f_3(x) - \frac{}{} b_1(x) - \frac{}{} b_2(x) = x^2 - \frac{\int_{-1}^1 x^2 1\ dx}{2} 1 - \frac{\int_{-1}^1 x^2 x\ dx}{2/3} x$ $b_3(x) = x^2 - \frac{2/3}{2} 1 - \frac{0}{2/3} x = x^2 - 1/3$

Step 3b: $o_3(x) = \frac{b_3(x)}{\|b_3(x)\|} = \frac{x^2-1/3}{\sqrt{}} = \frac{x^2-1/3}{\sqrt{\int_{-1}^1 (x^2-1/3)^2 dx}} = \frac{x^2-1/3}{\sqrt{\int_{-1}^1 x^4 - 2/3 x^2 + 1/9\ dx}}$ $o_3(x) = \frac{x^2-1/3}{\sqrt{8/45}} = \sqrt{\frac{5}{8}} (3x^2-1)$

It can be proven that $1/\sqrt{2}, x\sqrt{3/2}$ and $\sqrt{\frac{5}{8}} (3x^2-1)$ form a orthonormal basis with the above scalarproduct and norm.

### Numerical instability

Consider the vectors x1 = (1,ε,0,0),x2 = (1,0,ε,0) and x3 = (1,0,0,ε). Assume that ε is so small that computing 1 + ε = 1 holds on a computer (see http://en.wikipedia.org/wiki/Machine_epsilon). Let compute a orthonormal basis for this vectors in IR4 with the standard scalar product < x,y > = x1y1 + x2y2 + x3y3 + x4y4 and the norm $\|x\| = \sqrt{x_1^2+x_2^2+x_3^2+x_4^2}$.

Step 1a. b1 = x1 = (1,ε,0,0)

Step 1b. $o_1 = \frac{b_1}{\|b_1\|} = \frac{b_1}{\sqrt{1+\epsilon^2}} = b_1$ with 1 + ε2 = 1

Step 2a. $b_2 = x_2 - \frac{}{} b_1 = (1,0,\epsilon,0) - \frac{1}{1+\epsilon^2} (1,\epsilon,0,0) = (0,-\epsilon,\epsilon,0)$

Step 2b. $o_2 = \frac{b_2}{\|b_2\|} = \frac{b_2}{\sqrt{2\epsilon^2}} = (0,-\frac{1}{\sqrt{2}},\frac{1}{\sqrt{2}},0)$

Step 3a. $b_3 = x_3 - \frac{}{} b_1 - \frac{}{} b_2 = (1,0,0,\epsilon) - \frac{1}{1+\epsilon^2} (1,\epsilon,0,0) - \frac{0}{2\epsilon^2} (0,-\epsilon,\epsilon,0) = (0, -\epsilon, 0,\epsilon)$

Step 3b. $o_3 = \frac{b_3}{\|b_3\|} = \frac{b_3}{\sqrt{2\epsilon^2}} = (0,-\frac{1}{\sqrt{2}},0,\frac{1}{\sqrt{2}})$

It obvious that for the vectors

- $o_1 = (1, \epsilon, 0, 0)\$

- $o_2 = (0,-\frac{1}{\sqrt{2}},\frac{1}{\sqrt{2}},0)$

- $o_3 = (0,-\frac{1}{\sqrt{2}},0,\frac{1}{\sqrt{2}})$

the scalarproduct $ = 1/2 \neq 0$. All other pairs are also not zero, but they are multiplied with ε such that we get a result near zero.

### Modified Gram-Schmidt

To solve the problem a modified Gram-Schmidt algorithm is used:

1. Set bi = xi for all i
2. for each i from 1 to n compute
1. $o_i = \frac{b_i}{\|b_i\|}$
2. for each j from i + 1 to n compute $b_j = b_j - o_i\$

The difference is that we compute first our new bi and subtract it from all other bj. We apply the wrongly computed vector to all vectors instead of computing each bi separately.

### Example (recomputed)

Step 1. b1 = (1,ε,0,0), b2 = (1,0,ε,0), b3 = (1,0,0,ε)

Step 2a. $o_1 = \frac{b_1}{\|b_1\|} = \frac{b_1}{\sqrt{1+\epsilon^2}} = b_1 = (1,\epsilon,0,0)$ with 1 + ε2 = 1

Step 2b. $b_2 = b_2 - o_1 = (1,0,\epsilon,0) - (1,\epsilon,0,0) = (0, -\epsilon, \epsilon, 0)\$

Step 2c. $b_3 = b_3 - o_1 = (1,0,0,\epsilon) - (1,\epsilon,0,0) = (0, -\epsilon, 0, \epsilon)\$

Step 3a. $o_2 = \frac{b_2}{\|b_2\|} = \frac{b_2}{\sqrt{2\epsilon^2}} = (0,-\frac{1}{\sqrt{2}}, \frac{1}{\sqrt{2}}, 0)$

Step 3b. $b_3 = b_3 - o_2 = (0, -\epsilon, 0, \epsilon) - \frac{\epsilon}{\sqrt{2}} (0,-\frac{1}{\sqrt{2}}, \frac{1}{\sqrt{2}}, 0) = (0, -\epsilon/2, -\epsilon/2, \epsilon)$

Step 4a. $o_3 = \frac{b_3}{\|b_3\|} = \frac{b_3}{\sqrt{3/2\epsilon^2}} = (0,-\frac{1}{\sqrt{6}}, -\frac{1}{\sqrt{6}}, \frac{2}{\sqrt{6}})$

We can easily verify that < o2,o3 > = 0.

## Application

### Exploratory Project Pursuit

In the analysis of high-dimensional data we usually analyze projections of the data. The approach results from the Theorem of Cramer-Wold that states that the multidimensional distribution is fixed if we know all one-dimensional projections. Another theorem states that most (one-dimensional) projections of multivariate data are looking normal, even if the multivariate distribution of the data is highly non-normal.

Therefore in Exploratory Projection Pursuit we jugde the interestingness of a projection by comparison with a (standard) normal distribution. If we assume that the one-dimensional data x are standard normal distributed then after the transformation z = 2Φ − 1(x) − 1 with Φ(x) the cumulative distribution function of the standard normal distribution then z is uniformly distributed in the interval [ − 1;1].

Thus the interesting can measured by $\int_{-1}^1 (f(z)-1/2)^2 dx$ with f(z) a density estimated from the data. If the density f(z) is equal to 1 / 2 < math > inthein terval < math > [ − 1;1] then the integral becomes zero and we have found that our projected data are normally distributed. An value larger than zero indicates a deviation from the normal distribution of the projected data and hopefully an interesting distribution.

### Expansion with orthonormal polynomials

Let Li(z) a set of orthonormal polynomials with the scalar product $=\int_{-1}^1 f(z)g(z) dz$ and the norm $\|f\| = \sqrt{}$. What can we derive about a densities f(z) in the interval [ − 1;1] ?

If $f(z)=\sum_{i=0}^I a_i L_i(z)$ for some maximal degree I then it holds

$\int_{-1}^1 f(z) L_j(z) dz = \int_{-1}^1 \sum_{i=0}^I a_i L_i(z) L_j(z) dz = a_j \int_{-1}^1 L_j(z) L_j(z) dz = a_j$

We can also write $\int_{-1}^1 f(z) L_j(z) dz = E(L_j(z))$ or empirically we get an estimator $\hat{a}_j = \frac{1}{n} \sum_{k=1}^n L_j(z_k)$.

We describe the term $1/2 = \sum_{i=1}^I b_i L_i(z)$ and get for our integral

$\int_{-1}^1 (f(z)-1/2)^2 dz = \int_{-1}^1 \left(\sum_{i=0}^I (a_i-b_i) L_i(z)\right)^2 dz = \sum_{i,j=0}^I \int_{-1}^1 (a_i-b_i)(a_j-b_j) L_i(z) L_j(z) dz = \sum_{i=0}^I (a_i-b_i)^2.$

So using a orthonormal function set allows us to reduce the integral to a summation of coefficient which can be estimated from the data by plugging $\hat{a}_j$ in the formula above. The coefficients bi can be precomputed in advance.

### Normalized Legendre polynomials

The only problem left is to find the set of orthonormal polynomials Li(z) upto degree I. We know that 1,x,x2,...,x I form a basis for this space. We have to apply the Gram-Schmidt orthogonalization to find the orthonormal polynomials. This has been started in the first example.

The resulting polynomials are called normalized Legendre polynomials. Up to a sacling factor the normalized Legendre polynomials are identical to Legendre polynomials. The Legendre polynomials have a recursive expression of the form

$L_i(z) = \frac{(2i-1) L_{i-1}(z) - (i-1) L_{i-2}(z)}{i}$

So computing our integral reduces to computing L0(zk) and L1(zk) and using the recursive relationship to compute the $\hat{a}_j$'s. Please note that the recursion can be numerically unstable!

# Unconstrained Optimization

## Introduction

In the following we will provide some notes on numerical optimization algorithms. As there are numerous methods out there, we will restrict ourselves to the so-called Gradient Methods. There are basically two arguments why we consider this class as a natural starting point when thinking about numerical optimization algorithms. On the one hand, these methods are really workhorses in the field, so their frequent use in practice justifies their coverage here. On the other hand, this approach is highly intuitive in the sense that it somewhat follow naturally from the well-known properties of optima. In particular we will concentrate on three examples of this class: the Newtonian Method, the Method of Steepest Descent and the class of Variable Metric Methods, nesting amongst others the Quasi Newtonian Method.

Before we start we will nevertheless stress that there does not seem to be a "one and only" algorithm but the performance of specific algorithms is always contingent on the specific problem to be solved. Therefore both experience and "trial-and-error" are very important in applied work. To clarify this point we will provide a couple of applications where the performance of different algorithms can be compared graphically. Furthermore a specific example on Maximum Likelihood Estimation can be found at the end. Especially for statisticians and econometricians the Maximum Likelihood Estimator is probably the most important example of having to rely on numerical optimization algorithms in practice.

## Theoretical Motivation

Any numerical optimization algorithm has solve the problem of finding "observable" properties of the function such that the computer program knows that a solution is reached. As we are dealing with problems of optimization two well-known results seem to be sensible starting points for such properties.

If f is differentiable and $x^\star$ is a (local) minimum, then

$(1a) \quad Df(x^\star) = 0$

i.e. the Jacobian Df(x) is equal to zero

and

If f is twice differentiable and $x^\star$ is a (local) minimum, then

$(1b) \quad x^{T}D^2 f(x^\star)x \geq 0$

i.e. the Hessian D2f(x) is pos. semidefinite.

In the following we will always denote the minimum by $x^\star$. Although these two conditions seem to represent statements that help in finding the optimum $x^\star$, there is the little catch that they give the implications of $x^\star$ being an optimum for the function f. But for our purposes we would need the opposite implication, i.e. finally we want to arrive at a statement of the form: "If some condition $g(f(x^\star))$ is true, then $x^\star$ is a minimum". But the two conditions above are clearly not sufficient in achieving this (consider for example the case of f(x) = x3, with Df(0) = D2f(0) = 0 but $x^{\star} \neq 0$). Hence we have to look at an entire neighborhood of $x^\star$ as laid out in the following sufficient condition for detecting optima:

If $Df(x^\star) = 0$ and $x^{T}D^2f(z)x \geq 0, \forall x \in \mathbb{R}^n$ and $z \in \mathcal{B}(x^\star, \delta)$, then: $x^\star$ is a local minimum.

Proof: For $x \in \mathcal{B}(x^\star, \delta)$ let $z=x^\star + t(x-x^\star) \in \mathcal{B}$. The Taylor approximation yields: $f(x) - f(x^\star) = 0 + \frac{1}{2}(x-x^\star)^{T}D^2 f(z)(x-x^\star) \geq 0$, where $\mathcal{B}(x^\star, \delta)$ denotes an open ball around $x^\star$, i.e. $\mathcal{B}(x^\star, \delta) = \{x : ||x - x^\star|| \leq \delta \}$ for δ > 0.

In contrast to the two conditions above, this condition is sufficient for detecting optima - consider the two trivial examples

f(x) = x3 with $Df(x^\star = 0) = 0$ but $x^{T}D^2f(z)x = 6 z x^2 \not\geq 0 \quad (e.g. \,\,z = -\frac{\delta}{2})$

and

f(x) = x4 with $Df(x^\star = 0) = 0$ and $x^{T}D^2f(z)x = 12 z^2 x^2 \geq 0 \quad \forall z$.

Keeping this little caveat in mind we can now turn to the numerical optimization procedures.

## Numerical Solutions

All the following algorithms will rely on the following assumption:

(A1) The set $N(f,f(x^{(0)}) = \{x \in \mathbb{R}^n | f(x) \leq f(x^{(0)})\}$ is compact

where x(0) is some given starting value for the algorithm. The significance of this assumption has to be seen in the Weierstrass Theorem which states that every compact set contains its supremum and its infimum. So (A1) ensures that there is some solution in N(f,f(x(0)). And at this global minimum $x^\star$ it of course holds true that $D(f(x^\star)) = 0$. So - keeping the discussion above in mind - the optimization problem basically boils down to the question of solving set of equations $D(f(x^\star)) = 0$.

### The Direction of Descent

The problems with this approach are of course rather generically as $D(f(x^\star)) = 0$ does hold true for maxima and saddle points as well. Hence, good algorithms should ensure that both maxima and saddle points are ruled out as potential solutions. Maxima can be ruled out very easily by requiring f(x(k + 1)) < f(x(k)) i.e. we restrict ourselves to a sequence {x(k)}k such that the function value decreases in every step. The question is of course if this is always possible. Fortunately it is. The basic insight why this is the case is the following. When constructing the mapping $x^{(k+1)} = \varphi(x^{(k)})$ (i.e. the rule how we get from x(k) to x(k + 1)) we have two degrees of freedoms, namely

• the direction d(k) and
• the step length σ(k).

Hence we can choose in which direction we want to move to arrive at x(k + 1) and how far this movement has to be. So if we choose d(k) and σ(k) in the "right way" we can effectively ensure that the function value decreases. The formal representation of this reasoning is provided in the following

Lemma: If $d^{(k)} \in \mathbb{R}^n$ and Df(x)T d(k) < 0 then: $\exists \bar{\sigma} > 0$ such that

$f(x + \sigma^{(k)} d^{(k)}) < f(x) \quad \forall \sigma \in (0,\bar{\sigma})$

Proof: As Df(x)T d(k) < 0 and $Df(x)^{T} d^{(k)} = \lim_{\sigma \rightarrow 0} \frac{f(x + \sigma^{(k)} d^{(k)}) - f(x)}{\sigma^{(k)}}$, it follows that f(x + σ(k)d(k)) < f(x) for σ(k) small enough.

### The General Procedure of Descending Methods

A direction vector d(k) that satisfies this condition is is called a Direction of Descent. In practice this Lemma allows us to use the following procedure to numerically solve optimization problems.

1. Define the sequence {x(k)}k recursively via x(k + 1) = x(k) + σ(k)d(k)

2. Choose the direction d(k) from local information at the point x(k)

3. Choose a step size σ(k) that ensures convergence of the algorithm.

4. Stop the iteration if | f(x(k + 1)) − f(x(k)) | < ε where ε > 0 is some chosen tolerance value for the minimum

This procedure already hints that the choice of d(k) and σ(k) are not separable, but rather dependent. Especially note that even if the method is a descending method (i.e. both d(k) and σ(k) are chosen according to Lemma 1) the convergence to the minimum is not guaranteed. At a first glance this may seem a bit puzzling. If we found a sequence {x(k)}k such that the function value decreases at every step, one might think that at some stage, i.e. in the limit of k tending to infinity we should reach the solution. Why this is not the case can be seen from the following example borrowed from W. Alt (2002, p. 76).

#### Example 1

• Consider the following example which does not converge although it is clearly descending. Let the criterion function be given by

f(x) = x2, let the starting value be x(0) = 1, consider a (constant) direction vector d(k) = − 1 and choose a step width of $\sigma^{(k)} = (\frac{1}{2})^{k+2}$. Hence the recursive definition of the sequence {x(k)}k follows as

$(2) \quad x^{(k+1)} = x^{(k)} + (\frac{1}{2})^{k+2} (-1) = x^{(k-1)} - (\frac{1}{2})^{k+1} - (\frac{1}{2})^{k+2} = x^{(0)} - \sum_{j=0}^{k} (\frac{1}{2})^{j+2}.$

Note that $x^{(k)} > 0 \,\, \forall \,\, k$ and hence $f(x^{(k+1)}) < f(x^{(k)}) \,\, \forall \,\,k$, so that it is clearly a descending method. Nevertheless we find that

$(3) \quad lim_{k \rightarrow \infty}x^{(k)} = lim_{k \rightarrow \infty} x^{(0)} - \sum_{j=0}^{k-1} (\frac{1}{2})^{j+2} = lim_{k \rightarrow \infty} 1 - \frac{1}{4}(\frac{1-(\frac{1}{2})^{k}}{\frac{1}{2}}) = lim_{k \rightarrow \infty} \frac{1}{2} + (\frac{1}{2})^{k+1} = \frac{1}{2} \neq 0 = x^\star.$

The reason for this non-convergence has to be seen in the stepsize σ(k) decreasing too fast. For large k the steps x(k + 1)x(k) get so small that convergence is precluded. Hence we have to link the stepsize to the direction of descend d(k).

### Efficient Stepsizes

The obvious idea of such a linkage is to require that the actual descent is proportional to a first order approximation, i.e. to choose σ(k) such that there is a constant c1 > 0 such that

$(4) \quad f(x^{(k)} + \sigma^{(k)}d^{(k)}) - f(x^{(k)}) \leq c_1 \sigma^{(k)} D(f(x^{(k)})) d^{(k)} < 0.$

Note that we still look only at descending directions, so that Df(x(k)) Td(k) < 0 as required in Lemma 1 above. Hence, the compactness of N(f,f(x( k))) implies the convergence of the LHS and by (4)

$(5) \quad \lim_{k \rightarrow \infty} \sigma^{(k)} D(f(x^{(k)})) d^{(k)} = 0.$

Finally we want to choose a sequence {x(k)}k such that $\lim_{k \rightarrow \infty}D(f(x^{(k)})) = 0$ because that is exactly the necessary first order condition we want to solve. Under which conditions does (5) in fact imply $\lim_{k \rightarrow \infty}D(f(x^{(k)})) = 0$? First of all the stepsize σ(k) must not go to zero too quickly. That is exactly the case we had in the example above. Hence it seems sensible to bound the stepsize from below by requiring that

$(6) \quad \sigma^{(k)} \geq -c_{2} \frac{Df(x^{(k)})^{T}d^{(k)}}{|| d^{(k)}||^{2}} > 0$

for some constant c2 > 0. Substituting (6) into (5) finally yields

$(7) \quad f(x^{(k)} + \sigma^{(k)}d^{(k)}) - f(x^{(k)}) \leq -c (\frac{Df(x^{(k)})^{T}d^{(k)}}{|| d^{(k)}||})^{2}, \quad c = c_1 c_2$

where again the compactness of N(f,f(x( k))) ensures the convergence of the LHS and hence

$(8) \quad lim_{k \rightarrow \infty} -c (\frac{Df(x^{(k)})^{T}d^{(k)}}{|| d^{(k)}||})^{2} = lim_{k \rightarrow \infty} \frac{Df(x^{(k)})^{T}d^{(k)}}{|| d^{(k)}||} = 0$

Stepsizes that satisfy (4) and (6) are called efficient stepsizes and will be denoted by $\sigma_{E}^{(k)}$. The importance of condition (6) is illustated in the following continuation of Example 1.

#### Example 1 (continued)

• Note that it is exactly the failure of (6) that induced Exmaple 1 not to converge. Substituting the stepsize of the example into (6) yields

$(6.1) \quad \sigma^{(k)} = (\frac{1}{2})^{(k+2)} \geq -c_{2} \frac{2x^{(k)}(-1)}{1} = c_{2}\cdot2(\frac{1}{2}+(\frac{1}{2})^{k+1}) \Leftrightarrow \frac{1}{4(1+2^{(k)})} \geq c_{2} > 0$

so there is no constant c2 > 0 satisfying this inequality for all k as required in (6). Hence the stepsize is not bounded from below but decreases too fast. To really acknowledge the importance of (6), let us change the example a bit and assume that $\sigma^{(k)} = (\frac{1}{2})^{k+1}$. Then we find that

$(6.2) \quad lim_{k \rightarrow \infty} x^{(k+1)} = lim_{k \rightarrow \infty}x^{(0)} - \frac{1}{2}\sum_{i}(\frac{1}{2})^{i} = lim_{k \rightarrow \infty}(\frac{1}{2})^{k+1} = 0 = x^\star,$

i.e. convergence actually does take place. Furthermore recognize that this example actually does satisfy condition (6) as

$(6.3) \quad \sigma^{(k)} = (\frac{1}{2})^{(k+1)} \geq -c_{2} \frac{2x^{(k)}(-1)}{1} = c_{2}\cdot 2(\frac{1}{2})^{k} \Leftrightarrow \frac{1}{4} \geq c_{2} >0.$

### Choosing the Direction d

We have already argued that the choice of σ(k) and d(k) is intertwined. Hence the choice of the "right" d(k) is always contingent on the respective stepsize σ(k). So what does "right" mean in this context? Above we showed in equation (8) that choosing an efficient stepsize implied

$(8') \quad lim_{k \rightarrow \infty} -c (\frac{Df(x^{(k)})^{T}d^{(k)}}{|| d^{(k)}||})^{2} = lim_{k \rightarrow \infty} \frac{Df(x^{(k)})^{T}d^{(k)}}{|| d^{(k)}||} = 0.$

The "right" direction vector will therefore guarantee that (8') implies that

$(9) \quad lim_{k \rightarrow \infty} Df(x^{(k)}) = 0$

as (9) is the condition for the chosen sequence {x(k)}k to converge. So let us explore what directions could be chosen to yield (9). Assume that the stepsize σk is efficient and define

$(10) \quad \beta^{(k)} = \frac{Df(x^{(k)})^{T}d^{(k)}}{|| Df(x^{(k)})|| ||d^{(k)}||} \quad \Leftrightarrow \quad \beta^{(k)}|| Df(x^{(k)})|| = \frac{Df(x^{(k)})^{T}d^{(k)}}{|| d^{(k)}||}$

By (8') and (10) we know that

$(11) \quad lim_{k \rightarrow \infty} \beta^{(k)}|| Df(x^{(k)})|| = 0.$

So if we bound β(k) from below (i.e. $\beta^{(k)} \leq - \delta < 0$), (11) implies that

$(12) \quad lim_{k \rightarrow \infty} \beta^{(k)}|| Df(x^{(k)})|| = lim_{k \rightarrow \infty} || Df(x^{(k)})|| = lim_{k \rightarrow \infty} Df(x^{(k)}) = 0,$

where (12) gives just the condition of the sequence {x(k)}k converging to the solution $x^{\star}$. As (10) defines the direction vector d(k) implicitly by β(k), the requirements on β(k) translate directly into requirements on d(k).

When considering the conditions on β(k) it is clear where the term Gradient Methods originates from. With β(k) given by

$\beta_{k} = \frac{D(f(x)) d^{(k)}}{|| Df(x^{(k)}) || || d^{(k)} ||} = cos(Df(x^{(k)}),d^{(k)})$

we have the following result

Given that σ(k) was chosen efficiently and d(k) satisfies

$(13) \quad cos(Df(x^{(k)}),d^{(k)}) = \beta_{k} \leq - \delta < 0$

we have

$(14) \quad lim_{k \rightarrow \infty} Df(x^{(k)}) \rightarrow 0$

Hence: Convergence takes place if the angle between the negative gradient at x(k) and the direction d(k) is consistently smaller than the right angle. Methods relying on d(k) satisfying (13) are called Gradient Methods.

In other words: As long as one is not moving orthogonal to the gradient and if the stepsize is chosen efficiently, Gradient Methods guarantee convergence to the solution $x^{\star}$.

### Some Specific Algorithms in the Class of Gradient Methods

Let us now explore three specific algorithms of this class that differ in their respective choice of d(k).

#### The Newtonian Method

The Newtonian Method is by far the most popular method in the field. It is a well known method to solve for the roots of all types of equations and hence can be easily applied to optimization problems as well. The main idea of the Newtonian method is to linearize the system of equations to arrive at

$(15) \quad g(x) = g(\hat{x}) + Dg(\hat{x})^{T}(x-\hat{x}) = 0.$

(15) can easily be solved for x as the solution is just given by (assuming $Dg(\hat{x})^{T}$ to be non-singular)

$(16) \quad x = \hat{x} - [Dg(\hat{x})^{T}]^{-1}g(\hat{x}).$

For our purposes we just choose g(x) to be the gradient Df(x) and arrive at

$(17) \quad d_{N}^{(k)} = x^{(k+1)} - x^{(k)} = - [D^2f(x^{(k)})]^{-1}Df(x^{(k)})$

where $d_{N}^{(k)}$ is the so-called Newtonian Direction.

##### Properties of the Newtonian Method

Analyzing (17) elicits the main properties of the Newtonian method:

• If D2f(x( k)) is positive definite, $d_{N}^{k}$ is a direction of descent in the sense of Lemma 1.
• The Newtonian Method uses local information of the first and second derivative to calculate $d_{N}^{k}$.
• As

$(18) \quad x^{(k+1)} = x^{(k)} + d_{N}^{(k)}$

the Newtonian Method uses a fixed stepsize of σ(k) = 1. Hence the Newtonian method is not necessarily a descending method in the sense of Lemma 1. The reason is that the fixed stepsize σ(k) = 1 might be larger than the critical stepsize $\bar{\sigma_{k}}$ given in Lemma 1. Below we provide the Rosenbrock function as an example where the Newtonian Method is not descending.

• The Method can be time-consuming as calculating [D2f(x( k))] − 1 for every step k can be cumbersome. In applied work one could think about approximations. One could for example update the Hessian only every sth step or one could rely on local approximations. This is known as the Quasi-Newtonian-Method and will be discussed in the section about Variable Metric Methods.
• To ensure the method to be decreasing one could use an efficient stepsize $\sigma_{E}^{(k)}$ and set

$(19) \quad x^{(k+1)} = x^{(k)} - \sigma_{E}^{(k)}d_{N}^{(k)} = x^{(k)} - \sigma_{E}^{(k)} [D^2 f(x^{k})]^{-1} Df(x^{(k)})$

#### Method of Steepest Descent

Another frequently used method is the Method of Steepest Descent. The idea of this method is to choose the direction d(k) so that the decrease in the function value f is maximal. Although this procedure seems at a first glance very sensible, it suffers from the fact that it uses effectively less information than the Newtonian Method by ignoring the Hessian's information about the curvature of the function. Especially in the applications below we will see a couple of examples of this problem.

The direction vector of the Method of Steepest Descent is given by

$(20) \quad d_{SD}^{(k)} = argmax_{d : ||d|| = r} \{-Df(x^{(k)})^{T}d \} = argmin_{d : ||d|| = r} \{Df(x^{(k)})^{T}d \} = -r \frac{Df(x)}{|| Df(x) ||}$

Proof: By the Cauchy-Schwartz Inequality it follows that

$(21) \quad \frac{Df(x)^{T}d}{|| Df(x) || ||d||} \geq -1 \quad \Leftrightarrow \quad Df(x)^{T}d \geq -r || Df(x) ||.$

Obviously (21) holds with equality for $d^{(k)} = d_{SD}^{(k)}$ given in (20).

Note especially that for r = | | Df(x) | | we have $d_{SD}^{(k)} = - Df(x^{(k)})$, i.e. we just "walk" in the direction of the negative gradient. In contrast to the Newtonian Method the Method of Steepest Descent does not use a fixed stepsize but chooses an efficient stepsize $\sigma_{E}^{(k)}$. Hence the Method of Steepest Descent defines the sequence {x(k)}k by

$(22) \quad x^{(k+1)} = x^{(k)} + \sigma_{E}^{(k)} d_{SD}^{(k)},$

where $\sigma_{E}^{(k)}$ is an efficient stepsize and $d_{SD}^{(k)}$ the Direction of Steepest Descent given in (20).

##### Properties of the Method of Steepest Descent
• With $d_{SD}^{(k)} = -r \frac{Df(x)}{|| Df(x)||}$ the Method of Steepest Descent defines a direction of descent in the sense of Lemma 1, as

$Df(x)^{T}d_{SD}^{(k)} = Df(x)^{T}(-r \frac{Df(x)}{|| Df(x)||}) = - \frac{r}{|| Df(x)||}Df(x)^{T}Df(x) < 0.$

• The Method of Steepest Descent is only locally sensible as it ignores second order information.
• Especially when the criterion function is flat (i.e. the solution $x^\star$ lies in a "valley") the sequence defined by the Method of Steepest Descent fluctuates wildly (see the applications below, especially the example of the Rosenbrock function).
• As it does not need the Hessian, calculation and implementation of the Method of Steepest Descent is easy and fast.

#### Variable Metric Methods

A more general approach than both the Newtonian Method and the Method of Steepest Descent is the class of Variable Metric Methods. Methods in this class rely on the updating formula

$(23) \quad x^{k+1} = x^{k} - \sigma_{E}^{(k)} [A^{k}]^{-1} Df(x^{k}).$

If Ak is a symmetric and positive definite matrix, (23) defines a descending method as [Ak] − 1 is positive definite if and only if Ak is positive definite as well. To see this: just consider the spectral decomposition

$(24) \quad A^{k} = \Gamma \Lambda \Gamma^{T}$

where Γ and Λ are the matrices with eigenvectors and eigenvalues respectively. If Ak is positive definite, all eigenvalues λi are strictly positive. Hence their inverse $\lambda_{i}^{-1}$ are positive as well, so that [Ak] − 1 = ΓΛ − 1ΓT is clearly positive definite. But then, substitution of d(k) = [Ak] − 1Df(xk) yields

$(25) \quad Df(x^{k})^{T}d^{(k)} = -Df(x^{k})^{T}[A^{k}]^{-1}Df(x^{k}) \equiv - v^{T} [A^{k}]^{-1} v \leq 0,$

i.e. the method is indeed descending. Up to now we have not specified the matrix Ak, but is easily seen that for two specific choices, the Variable Metric Method just coincides with the Method of Steepest Descent and the Newtonian Method respectively.

• For $A^{k} = \mathcal{I}$ (with $\mathcal{I}$ being the identity matrix) it follows that

$(22') \quad x^{k+1} = x^{k} - \sigma_{E}^{(k)} Df(x^{k})$

which is just the Method of Steepest Descent.

• For Ak = D2f(xk) it follows that

$(19') \quad x^{k+1} = x^{k} - \sigma_{E}^{(k)} [D^{2}f(x^{k})]^{-1}Df(x^{k})$

which is just the Newtonian Method using a stepsize $\sigma_{E}^{(k)}$.

##### The Quasi Newtonian Method

A further natural candidate for a Variable Metric Method is the Quasi Newtonian Method. In contrast to the standard Newtonian Method it uses an efficient stepsize so that it is a descending method and in contrast to the Method of Steepest Descent it does not fully ignore the local information about the curvature of the function. Hence the Quasi Newtonian Method is defined by the two requirements on the matrix Ak:

• Ak should approximate the Hessian D2f(x k) to make use of the information about the curvature and
• the update $A^{k} \rightarrow A^{k+1}$ should be easy so that the algorithm is still relatively fast (even in high dimensions).

To ensure the first requirement, Ak + 1 should satisfy the so-called Quasi-Newtonian-Equation

$(26) \quad A^{k+1}(x^{(k+1)} - x^{(k)}) = Df(x^{(k+1)})-Df(x^{(k)})$

as all Ak satisfying (26) reflect information about the Hessian. To see this, consider the function g(x) defined as

$(27) \quad g(x) = f(x^{k+1})+Df(x^{k+1})^{T}(x - x^{k+1})+\frac{1}{2}(x-x^{k+1})^{T}A^{k+1}(x - x^{k+1}).$

Then it is obvious that g(xk + 1) = f(xk + 1) and Dg(xk + 1) = Df(xk + 1). So g(x) and f(x) are reasonably similar in the neighborhood of x(k + 1). In order to ensure that g(x) is also a good approximation at x(k), we want to choose Ak + 1 such that the gradients at x(k) are identical. With

$(28) \quad Dg(x^{k}) = Df(x^{k+1}) - A^{k+1} (x^{k+1} - x^{k})$

it is clear that Dg(xk) = Df(xk) if Ak + 1 satisfies the Quasi Newtonian Equation given in (26). But then it follows that

$(29) \quad A^{k+1} (x^{k+1} - x^{k}) = Df(x^{k+1}) - Dg(x^{k}) = Df(x^{k+1}) - Df(x^{k}) = D^2 f(\lambda x^{(k)} + (1-\lambda)x^{(k+1)})(x^{k+1} - x^{k}).$

Hence as long as x(k + 1) and x(k) are not too far apart, Ak + 1 satisfying (26) is a good approximation of D2f(x( k)).

Let us now come to the second requirement that the update of the Ak should be easy. One specific algorithm to do so is the so-called BFGS-Algorithm. The main merit of this algorithm is the fact that it uses only the already calculated elements {x(k)}k and {Df(x(k))} k to construct the update A(k + 1). Hence no new entities have to be calculated but one has only to keep track of the x-sequence and sequence of gradients. As a starting point for the BFGS-Algorithm one can provide any positive definite matrix (e.g. the identity matrix or the Hessian at x(0)). The BFGS-Updating-Formula is then given by

$(30) \quad A^{k} = A^{k-1} - \frac{(A^{k-1})^{T}\gamma_{k-1}^{T}\gamma_{k-1}A^{k-1}}{\gamma_{k-1}^{T}A^{k-1}\gamma_{k-1}} + \frac{\Delta_{k-1}\Delta_{k-1}^{T}}{\Delta_{k-1}^{T}\gamma_{k-1}}$

where Δk − 1 = Df(x(k)) − Df(x(k − 1)) and γk − 1 = x(k)x(k − 1). Furthermore (30) ensures that all Ak are positive definite as required by Variable Metric Methods to be descending.

##### Properties of the Quasi Newtonian Method
• It uses second order information about the curvature of f(x) as the matrices Ak are related to the Hessian D2f(x).
• Nevertheless it ensures easy and fast updating (e.g. by the BFGS-Algorithm) so that it is faster than the standard Newtonian Method.
• It is a descending method as Ak are positive definite.
• It is relatively easy to implement as the BFGS-Algorithm is available in most numerical or statistical software packages.

## Applications

To compare the methods and to illustrate the differences between the algorithms we will now evaluate the performance of the Steepest Descent Method, the standard Newtonian Method and the Quasi Newtonian Method with an efficient stepsize. We use two classical functions in this field, namely the Himmelblau and the Rosenbrock function.

### Application I: The Himmelblau Function

The Himmelblau function is given by

$(31) \quad f(x,y) = (x^2 + y - 11)^2 + (x + y^2 - 7)^2$

This fourth order polynomial has four minima, four saddle points and one maximum so there are enough possibilities for the algorithms to fail. In the following pictures we display the contour plot and the 3D plot of the function for different starting values.

In Figure 1 we display the function and the paths of all three methods at a starting value of (2, − 4). Obviously the three methods do not find the same minimum. The reason is of course the different direction vector of the Method of Steepest Descent - by ignoring the information about the curvature it chooses a totally different direction than the two Newtonian Methods (see especially the right panel of Figure 1).

Figure 1: The two Newton Methods converge to the same, the Method of Steepest Descent to a different minimum.

Consider now the starting value (4.5, − 0.5), displayed in Figure 2. The most important thing is of course that now all methods find different solutions. That the Method of Steepest Descent finds a different solution than the two Newtonian Methods is again not that suprising. But that the two Newtonian Methods converge to different solution shows the significance of the stepsize σ. With the Quasi-Newtonian Method choosing an efficient stepsize in the first iteration, both methods have different stepsizes and direction vectors for all iterations after the first one. And as seen in the picture: the consequence may be quite significant.

Figure 2: Even all methods find different solutions.

### Application II: The Rosenbrock Function

The Rosenbrock function is given by

$(32) \quad f(x,y) = 100(y - x^2)^2 + (1-x)^2 \$

Although this function has only one minimum it is an interesting function for optimization problems. The reason is the very flat valley of this U-shaped function (see the right panels of Figures 3 and 4). Especially for econometricians this function may be interesting because in the case of Maximum Likelihood estimation flat criterion functions occur quite frequently. Hence the results displayed in Figures 3 and 4 below seem to be rather generic for functions sharing this problem.

My experience when working with this function and the algorithms I employed is that Figure 3 (given a starting value of (2, − 5)) seems to be quite characteristic. In contrast to the Himmelblau function above, all algorithms found the same solution and given that there is only one minimum this could be expected. More important is the path the different methods choose as is reflects the different properties of the respective methods. It is seen that the Method of Steepest Descent fluctuates rather wildly. This is due to the fact that it does not use information about the curvature but rather jumps back and forth between the "hills" adjoining the valley. The two Newtonian Methods choose a more direct path as they use the second order information. The main difference between the two Newtonian Methods is of course the stepsize. Figure 3 shows that the Quasi Newtonian Method uses very small stepsizes when working itself through the valley. In contrast, the stepsize of the Newtonian Method is fixed so that it jumps directly in the direction of the solution. Although one might conclude that this is a disadvantage of the Quasi Newtonian Method, note of course that in general these smaller stepsizes come with benefit of a higher stability, i.e. the algorithm is less likely to jump to a different solution. This can be seen in Figure 4.

Figure 3: All methods find the same solution, but the Method of Steepest Descent fluctuates heavily.

Figure 4, which considers a starting value of ( − 2, − 2), shows the main problem of the Newtonian Method using a fixed stepsize - the method might "overshoot" in that it is not descending. In the first step, the Newtonian Method (displayed as the purple line in the figure) jumps out of the valley to only bounce back in the next iteration. In this case convergence to the minimum still occurs as the gradient at each side points towards the single valley in the center, but one can easily imagine functions where this is not the case. The reason of this jump are the second derivatives which are very small so that the step [Df(x(k))] − 1Df(x(k))) gets very large due to the inverse of the Hessian. In my experience I would therefore recommend to use efficient stepsizes to have more control over the paths the respective Method chooses.

Figure 2: Overshooting of the Newtonian Method due to the fixed stepsize.

### Application III: Maximum Likelihood Estimation

For econometricians and statisticians the Maximum Likelihood Estimator is probably the most important application of numerical optimization algorithms. Therefore we will briefly show how the estimation procedure fits in the framework developed above.

As usual let

$(33) \quad f(Y | X; \theta)$

be the conditional density of Y given X with parameter θ and

$(34) \quad l(\theta; Y | X)$

the conditional likelihood function for the parameter θ

If we assume the data to be independently, identically distributed (iid) then the sample log-likelihood follows as

$(35) \quad \mathcal{L}(\theta; Y_{1}, ..., Y_{N}) = \sum_{i}^{N} \mathcal{L}(\theta; Y_{i}) = \sum_{i}^{N} log(l(\theta; Y_{i})).$

Maximum Likelihood estimation therefore boils down to maximize (35) with respect to the parameter θ. If we for simplicity just decide to use the Newtonian Method to solve that problem, the sequence (k)}k is recursively defined by

$(36) \quad D_{\theta}\mathcal{L}(\theta^{(k+1)}) = D_{\theta}\mathcal{L}(\theta^{(k)}) + D_{\theta \theta}\mathcal{L}(\theta^{(k)})(\theta^{(k+1)} -\theta^{(k)}) = 0 \Leftrightarrow \theta^{(k+1)} = \theta^{(k)} - [D_{\theta \theta}\mathcal{L}(\theta^{(k)})]^{-1}D_{\theta}\mathcal{L}(\theta^{(k)})$

where $D_{\theta}\mathcal{L}$ and $D_{\theta \theta}\mathcal{L}$ denotes the first and second derivative with respect to the parameter vector θ and $[D_{\theta \theta} \mathcal{L}(\theta^{(k)})]^{-1}D_{\theta} \mathcal{L}(\theta^{(k)})$ defines the Newtonian Direction given in (17). As Maximum Likelihood estimation always assumes that the conditional density (i.e. the distribution of the error term) is known up to the parameter θ, the methods described above can readily be applied.

#### A Concrete Example of Maximum Likelihood Estimation

Assume a simple linear model

$(37a) \quad Y_{i} = \beta_{1} + \beta_{x} X_{i} + U_{i}$

with θ = (β12)'. The conditional distribution Y is then determined by the one of U, i.e.

$(37b) \quad p(Y_{i} - \beta_{1} - \beta_{x} X_{i}) \equiv p_{\mid X_{i}}(Y_{i}) = p(U_{i}),$

where p denotes the density function. Generally, there is no closed form solution of maximizing (35) (at least if U does not happen to be normally distributed), so that numerical methods have to be employed. Hence assume that U follows Student's t-distribution with m degrees of freedom so that (35) is given by

$(38) \quad \mathcal{L}(\theta;Y_{\mid X}) = \sum log( \frac{\Gamma(\frac{m+1}{2})}{\sqrt{\pi m}\Gamma(\frac{m}{2})}(1+\frac{(y_{i} - x_{i}^{T}\beta)^2}{m})^{-\frac{m+1}{2}})$

where we just used the definition of the density function of the t-distribution. (38) can be simplified to

$(39) \quad \mathcal{L}(\theta;Y_{\mid X}) = N[log(\Gamma(\frac{m+1}{2})) - log(\sqrt{\pi m}\Gamma(\frac{m}{2}))] -\frac{m+1}{2} \sum log(1+\frac{(y_{i} - x_{i}^{T}\beta)^2}{m})$

so that (if we assume that the degrees of freedom m are known)

$(40) \quad \textit{argmax} \{ \mathcal{L}(\theta;Y_{\mid X}) \} = \textit{argmax} \{ -\frac{m+1}{2} \sum log(1+\frac{(y_{i} - x_{i}^{T}\beta)^2}{m}) \} = \textit{argmin} \{ \sum log(1+\frac{(y_{i} - x_{i}^{T}\beta)^2}{m}) \}.$

With the criterion function

$(41) \quad f(\beta_{1}, \beta_{2}) = \sum log(1+\frac{(y_{i} - \beta_{1} - \beta_{2}x_{i})^2}{m})$

the methods above can readily applied to calculate the Maximum Likelihood Estimator $(\hat{\beta}_{1,ML}, \hat{\beta}_{2,ML})$ maximizing (41).

## References

• Alt, W. (2002): "Nichtlineare Optimierung", Vieweg: Braunschweig/Wiesbaden
• Härdle, W. and Simar, L. (2003): "Applied Multivariate Statistical Analysis", Springer: Berlin Heidelberg
• Königsberger, K. (2004): "Analysis I", Springer: Berlin Heidelberg
• Ruud, P. (2000): "Classical Econometric Theory", Oxford University Press: New York

# Quantile Regression

Quantile Regression as introduced by Koenker and Bassett (1978) seeks to complement classical linear regression analysis. Central hereby is the extension of "ordinary quantiles from a location model to a more general class of linear models in which the conditional quantiles have a linear form" (Buchinsky (1998), p. 89). In Ordinary Least Squares (OLS) the primary goal is to determine the conditional mean of random variable Y, given some explanatory variable xi, reaching the expected value E[Y | xi]. Quantile Regression goes beyond this and enables one to pose such a question at any quantile of the conditional distribution function. The following seeks to introduce the reader to the ideas behind Quantile Regression. First, the issue of quantiles is addressed, followed by a brief outline of least squares estimators focusing on Ordinary Least Squares. Finally, Quantile Regression is presented, along with an example utilizing the Boston Housing data set.

## Preparing the Grounds for Quantile Regression

### What are Quantiles

Gilchrist (2001, p.1) describes a quantile as "simply the value that corresponds to a specified proportion of an (ordered) sample of a population". For instance a very commonly used quantile is the median M, which is equal to a proportion of 0.5 of the ordered data. This corresponds to a quantile with a probability of 0.5 of occurrence. Quantiles hereby mark the boundaries of equally sized, consecutive subsets. (Gilchrist, 2001)

More formally stated, let Y be a continuous random variable with a distribution function FY(y) such that

$(1) F_Y(y) = P (Y\leq {y}) = \tau$

which states that for the distribution function FY(y) one can determine for a given value y the probability τ of occurrence. Now if one is dealing with quantiles, one wants to do the opposite, that is one wants to determine for a given probability τ of the sample data set the corresponding value y. A τth quantile refers in a sample data to the probability τ for a value y.

(2)FY(yτ) = τ

Another form of expressing the τth quantile mathematically is following:

$(3) y_\tau = F_{Y}^{-1}(\tau)$

yτ is such that it constitutes the inverse of the function FY(τ) for a probability τ.

Note that there are two possible scenarios. On the one hand, if the distribution function FY(y) is monotonically increasing, quantiles are well defined for every $\tau \in (0;1)$. However, if a distribution function FY(y) is not strictly monotonically increasing , there are some τs for which a unique quantile can not be defined. In this case one uses the smallest value that y can take on for a given probability τ.

Both cases, with and without a strictly monotonically increasing function, can be described as follows:

$(4) y_\tau = F_Y^{-1}(\tau) = inf \left\{ y | F_Y(y) \geq \tau \right\}$

That is yτ is equal to the inverse of the function FY(τ) which in turn is equal to the infimum of y such that the distribution function FY(y) is greater or equal to a given probability τ, i.e. the τth quantile. (Handl (2000))

However, a problem that frequently occurs is that an empirical distribution function is a step function. Handl (2000) describes a solution to this problem. As a first step, one reformulates equation 4 in such a way that one replaces the continuous random variable Y with n, the observations, in the distribution function FY(y), resulting in the empirical distribution function Fn(y). This gives the following equation:

$(5) \hat{y}_\tau = inf \left\{ y | F_n(y) \geq \tau \right\}$

The empirical distribution function can be separated into equally sized, consecutive subsets via the the number of observations n. Which then leads one to the following step:

$(6) \hat{y}_\tau = y_{(i)}$

with i = 1,...,n and y(1),...,y(n) as the sorted observations. Hereby, of course, the range of values that yτ can take on is limited simply by the observations y(i) and their nature. However, what if one wants to implement a different subset, i.e. different quantiles but those that can be derived from the number of observations n?

Therefore a further step necessary to solving the problem of a step function is to smooth the empirical distribution function through replacing it a with continuous linear function $\tilde{F}(y)$. In order to do this there are several algorithms available which are well described in Handl (2000) and more in detail with an evaluation of the different algorithms and their efficiency in computer packages in Hyndman and Fan (1996). Only then one can apply any division into quantiles of the data set as suitable for the purpose of the analysis. (Handl (2000))

### Ordinary Least Squares

In regression analysis the researcher is interested in analyzing the behavior of a dependent variable yi given the information contained in a set of explanatory variables xi. Ordinary Least Squares is a standard approach to specify a linear regression model and estimate its unknown parameters by minimizing the sum of squared errors. This leads to an approximation of the mean function of the conditional distribution of the dependent variable. OLS achieves the property of BLUE, it is the best, linear, and unbiased estimator, if following four assumptions hold:

1. The explanatory variable xi is non-stochastic

2. The expectations of the error term εi are zero, i.e. Ei] = 0

3. Homoscedasticity - the variance of the error terms εi is constant, i.e. vari) = σ2

4. No autocorrelation, i.e. covi j) = 0 , $i\neq j$

However, frequently one or more of these assumptions are violated, resulting in that OLS is not anymore the best, linear, unbiased estimator. Hereby Quantile Regression can tackle following issues: (i), frequently the error terms are not necessarily constant across a distribution thereby violating the axiom of homoscedasticity. (ii) by focusing on the mean as a measure of location, information about the tails of a distribution are lost. (iii) OLS is sensitive to extreme outliers that can distort the results significantly. (Montenegro (2001))

## Quantile Regression

### The Method

Quantile Regression essentially transforms a conditional distribution function into a conditional quantile function by slicing it into segments. These segments describe the cumulative distribution of a conditional dependent variable Y given the explanatory variable xi with the use of quantiles as defined in equation 4.

For a dependent variable Y given the explanatory variable X = x and fixed τ, 0 < τ < 1, the conditional quantile function is defined as the τ − th quantile QY | X(τ | x) of the conditional distribution function FY | X(y | x). For the estimation of the location of the conditional distribution function, the conditional median QY | X(0,5 | x) can be used as an alternative to the conditional mean. (Lee (2005))

One can nicely illustrate Quantile Regression when comparing it with OLS. In OLS, modeling a conditional distribution function of a random sample (y1,...,yn) with a parametric function μ(xi,β) where xi represents the independent variables, β the corresponding estimates and μ the conditional mean, one gets following minimization problem:

$(7) min_{\beta\in\Re}\sum_{i=1}^{n}(y_i-\mu(x_i,\beta))^{2}$

One thereby obtains the conditional expectation function E[Y | xi]. Now, in a similar fashion one can proceed in Quantile Regression. Central feature thereby becomes ρτ, which serves as a check function.

$(8) \rho_{\tau}(x)=\begin{cases}\tau*x & \mbox{if } x \ge 0 \\ (\tau-1)*x & \mbox{if } x < 0 \end{cases}$

This check-function ensures that

1. all ρτ are positive

2. the scale is according to the probability τ

Such a function with two supports is a must if dealing with L1 distances, which can become negative.

In Quantile Regression one minimizes now following function:

$(9) min_{\beta\in\Re}\sum_{i=1}^{n}\rho_{\tau}(y_i-\xi(x_i,\beta))$

Here, as opposed to OLS, the minimization is done for each subsection defined by ρτ, where the estimate of the τth-quantile function is achieved with the parametric function ξ(xi,β). (Koenker and Hallock (2001))

Features that characterize Quantile Regression and differentiate it from other regression methods are following:

1. The entire conditional distribution of the dependent variable Y can be characterized through different values of τ

2. Heteroscedasticity can be detected

3. If the data is heteroscedastic, median regression estimators can be more efficient than mean regression estimators

4. The minimization problem as illustrated in equation 9 can be solved efficiently by linear programming methods, making estimation easy

5. Quantile functions are also equivariant to monotone transformations. That is Qh(Y | X)(xτ) = h(Q(Y | X)(xτ)), for any function

6. Quantiles are robust in regards to outliers ( Lee (2005) )

### A graphical illustration of Quantile Regression

Before proceeding to a numerical example, the following subsection seeks to graphically illustrate the concept of Quantile Regression. First, as a starting point for this illustration, consider figure 1. For a given explanatory value of xi the density for a conditional dependent variable Y is indicated by the size of the balloon. The bigger the balloon, the higher is the density, with the mode, i.e. where the density is the highest, for a given xi being the biggest balloon. Quantile Regression essentially connects the equally sized balloons, i.e. probabilities, across the different values of xi, thereby allowing one to focus on the interrelationship between the explanatory variable xi and the dependent variable Y for the different quantiles, as can be seen in figure 2. These subsets, marked by the quantile lines, reflect the probability density of the dependent variable Y given xi.

Figure 1: Probabilities of occurrence for individual explanatory variables

The example used in figure 2 is originally from Koenker and Hallock (2000), and illustrates a classical empirical application, Ernst Engel's (1857) investigation into the relationship of household food expenditure, being the dependent variable, and household income as the explanatory variable. In Quantile Regression the conditional function of QY | X(τ | x) is segmented by the τth-quantile. In the analysis, the τth-quantiles $\tau \in\left\{0,05; 0,1; 0,25; 0,5; 0,75; 0,9; 0,95\right\}$, indicated by the thin blue lines that separate the different color sections, are superimposed on the data points. The conditional median (τ = 0,5) is indicated by a thick dark blue line, the conditional mean by a light yellow line. The color sections thereby represent the subsections of the data as generated by the quantiles.

Figure 2: Engels Curve, with the median highlighted in dark blue and the mean in yellow

Figure 2 can be understood as a contour plot representing a 3-D graph, with food expenditure and income on the respective y and x axis. The third dimension arises from the probability density of the respective values. The density of a value is thereby indicated by the darkness of the shade of blue, the darker the color, the higher is the probability of occurrence. For instance, on the outer bounds, where the blue is very light, the probability density for the given data set is relatively low, as they are marked by the quantiles 0,05 to 0,1 and 0,9 to 0,95. It is important to notice that figure 2 represents for each subsections the individual probability of occurrence, however, quantiles utilize the cumulative probability of a conditional function. For example, τ of 0,05 means that 5$\%$ of observations are expected to fall below this line, a τ of 0,25 for instance means that 25$\%$ of the observations are expected to fall below this and the 0,1 line.

The graph in figure 2, suggests that the error variance is not constant across the distribution. The dispersion of food expenditure increases as household income goes up. Also the data is skewed to the left, indicated by the spacing of the quantile lines that decreases above the median and also by the relative position of the median which lies above the mean. This suggests that the axiom of homoscedasticity is violated, which OLS relies on. The statistician is therefore well advised to engage in an alternative method of analysis such as Quantile Regression, which is actually able to deal with heteroscedasticity.

### A Quantile Regression Analysis

In order to give a numerical example of the analytical power of Quantile Regression and to compare it within the boundaries of a statistical application with OLS the following section will be analyzing some selected variables of the Boston Housing dataset which is available at the md-base website. The data was first analyzed by Belsley, Kuh, and Welsch (1980). The original data comprised 506 observations for 14 variables stemming from the census of the Boston metropolitan area.

This analysis utilizes as the dependent variable the median value of owner occupied homes (a metric variable, abbreviated with H) and investigates the effects of 4 independent variables as shown in table 1. These variables were selected as they best illustrate the difference between OLS and Quantile Regression. For the sake of simplicity of the analysis, it was neglected for now to deal with potential difficulties related to finding the correct specification of a parametric model. A simple linear regression model therefore was assumed. For the estimation of asymptotic standard errors see for example Buchinsky (1998), which illustrates the design-matrix bootstrap estimator or alternatively Powell (1986) for kernel based estimation of asymptotic standard errors.

Table1: The explanatory variables
Name Short What it is type
NonrTail T Proportion of non-retail business acres metric
NoorOoms O Average number of rooms per dwelling metric
Age A Proportion of owner-built dwellings prior to 1940 metric
PupilTeacher P Pupil-teacher ratio metric

In the following firstly an OLS model was estimated. Three digits after the comma were indicated in the tables as some of the estimators turned out to be very small.

(10)E[Hi | Ti,Oi, Ai,Pi] = α + βTi + δOi + γAi + λPi

Computing this via XploRe one obtains the results as shown in the table below.

Table2: OLS estimates
$\hat{\alpha}$ $\hat{\beta}$ $\hat{\delta}$ $\hat{\gamma}$ $\hat{\lambda}$
36,459 0,021 38,010 0,001 -0,953

Analyzing this data set via Quantile Regression, utilizing the τth quantiles $\tau \in \left(0,1; 0,3; 0,5; 0,7; 0,9\right)$ the model is characterized as follows:

(11)QH[τ | Ti,Oi, Ai,Pi] = ατ + βτTi + δτOi + γτAi + λτPi

Just for illustrative purposes and to further foster the understanding of the reader for Quantile Regression, the equation for the 0,1th quantile is briefly illustrated, all others follow analogous:

$(12) min\left[\rho_{0,1}(y_1-x_1\beta)+\rho_{0,1}(y_2-x_2\beta)+ ...+\rho_{0,1}(y_n-x_n\beta)\right]$

$\mbox{ equation 12 with } \rho_{0,1}(y_i-x_i\beta)=\begin{cases}0,1(y_i-x_i\beta) & \mbox{if }(y_i-x_i\beta)>0 \\-0,9(y_i-x_i\beta) & \mbox{if }(y_i-x_i\beta)<0 \end{cases}$

Table3: Quantile Regression estimates
τ $\hat{\alpha}_\tau$ $\hat{\beta}_\tau$ $\hat{\delta}_\tau$ $\hat{\gamma}_\tau$ $\hat{\lambda}_\tau$
0,1 23,442 0,087 29,606 -0,022 -0,443
0,3 15,7130 -0,001 45,281 -0,037 -0,617
0,5 14,8500 0,022 53,252 -0,031 -0,737
0,7 20,7910 -0,021 50,999 -0,003 -0,925
0,9 34,0310 -0,067 51,353 0,004 -1,257

Now if one compares the results for the estimates of OLS from table 2 and Quantile Regression, table 3, one finds that the latter method can make much more subtle inferences of the effect of the explanatory variables on the dependent variable. Of particular interest are thereby quantile estimates that are relatively different as compared to other quantiles for the same estimate.

Probably the most interesting result and most illustrative in regards to an understanding of the functioning of Quantile Regression and pointing to the differences with OLS are the results for the independent variable of the proportion of non-retail business acres (Ti). OLS indicates that this variable has a positive influence on the dependent variable, the value of homes, with an estimate of $\hat{\beta}=0,021$, i.e. the value of houses increases as the proportion of non-retail business acres (Ti) increases in regards to the Boston Housing data.

Looking at the output that Quantile Regression provides us with, one finds a more differentiated picture. For the 0,1 quantile, we find an estimate of $\hat{\beta}_{0,1}= 0,087$ which would suggest that for this low quantile the effect seems to be even stronger than is suggested by OLS. Here house prices go up when the proportion of non-retail businesses (Ti) goes up, too. However, considering the other quantiles, this effect is not quite as strong anymore, for the 0,7th and 0,9th quantile this effect seems to be even reversed indicated by the parameter $\hat{\beta}_{0,7}= -0,021$ and $\hat{\beta}_{0,9}= -0,062$. These values indicate that in these quantiles the house price is negatively influenced by an increase of non-retail business acres (Ti). The influence of non-retail business acres (Ti) seems to be obviously very ambiguous on the dependent variable of housing price, depending on which quantile one is looking at. The general recommendation from OLS that if the proportion of non-retail business acres (Ti) increases, the house prices would increase can obviously not be generalized. A policy recommendation on the OLS estimate could therefore be grossly misleading.

One would intuitively find the statement that the average number of rooms of a property (Oi) positively influences the value of a house, to be true. This is also suggested by OLS with an estimate of $\hat{\delta}=38,099$. Now Quantile Regression also confirms this statement, however, it also allows for much subtler conclusions. There seems to be a significant difference between the 0,1 quantile as opposed to the rest of the quantiles, in particular the 0,9th quantile. For the lowest quantile the estimate is $\hat{\delta}_{0,1}= 29,606$, whereas for the 0,9th quantile it is $\hat{\delta}_{0,9}=51,353$. Looking at the other quantiles one can find similar values for the Boston housing data set as for the 0,9th, with estimates of $\hat{\delta}_{0,3}=45,281$, $\hat{\delta}_{0,5}=53,252$, and $\hat{\delta}_{0,7}=50,999$ respectively. So for the lowest quantile the influence of additional number of rooms (Oi) on the house price seems to be considerably smaller then for all the other quantiles.

Another illustrative example is provided analyzing the proportion of owner-occupied units built prior to 1940 (Ai) and its effect on the value of homes. Whereas OLS would indicate this variable has hardly any influence with an estimate of $\hat{\gamma}=0,001$, looking at Quantile Regression one gets a different impression. For the 0,1th quantile, the age has got a negative influence on the value of the home with $\hat{\gamma}_{0,1}=-0,022$. Comparing this with the highest quantile where the estimate is $\hat{\gamma}_{0,9}=0,004$, one finds that the value of the house is suddenly now positively influenced by its age. Thus, the negative influence is confirmed by all other quantiles besides the highest, the 0,9th quantile.

Last but not least, looking at the pupil-teacher ratio (Pi) and its influence on the value of houses, one finds that the tendency that OLS indicates with a value of $\hat{\lambda}=-0,953$ to be also reflected in the Quantile Regression analysis. However, in Quantile Regression one can see that the influence on the housing price of the pupils-teacher ratio (Pi) gradually increases over the different quantiles, from the 0,1th quantile with an estimate of $\hat{\lambda}_{0,1}=-0,443$ to the 0,9th quantile with a value of $\hat{\lambda}_{0,9}=-1,257$.

This analysis makes clear, that Quantile Regression allows one to make much more differentiated statements when using Quantile Regression as opposed to OLS. Sometimes OLS estimates can even be misleading what the true relationship between an explanatory and a dependent variable is as the effects can be very different for different subsection of the sample.

## Conclusion

For a distribution function FY(y) one can determine for a given value of y the probability τ of occurrence. Now quantiles do exactly the opposite. That is, one wants to determine for a given probability τ of the sample data set the corresponding value y. In OLS, one has the primary goal of determining the conditional mean of random variable Y, given some explanatory variable xi , E[Y | xi]. Quantile Regression goes beyond this and enables us to pose such a question at any quantile of the conditional distribution function. It focuses on the interrelationship between a dependent variable and its explanatory variables for a given quantile. Quantile Regression overcomes thereby various problems that OLS is confronted with. Frequently, error terms are not constant across a distribution, thereby violating the axiom of homoscedasticity. Also, by focusing on the mean as a measure of location, information about the tails of a distribution are lost. And last but not least, OLS is sensitive to extreme outliers, which can distort the results significantly. As has been indicated in the small example of the Boston Housing data, sometimes a policy based upon an OLS analysis might not yield the desired result as a certain subsection of the population does not react as strongly to this policy or even worse, responds in a negative way, which was not indicated by OLS.

## References

Abrevaya, J. (2001): “The effects of demographics and maternal behavior on the distribution of birth outcomes,” in Economic Application of Quantile Regression, ed. by B. Fitzenberger, R. Koenker, and J. A. Machade, pp. 247–257. Physica-Verlag Heidelberg, New York.

Belsley, D. A., E. Kuh, and R. E. Welsch (1980): Applied Multivariate Statistical Analysis. Regression Diagnostics, Wiley.

Buchinsky, M. (1998): “Recent Advances in Quantile Regression Models: A Practical Guidline for Empirical Research,” Journal of Human Resources, 33(1), 88–126.

Cade, B.S. and B.R. Noon (2003): A gentle introduction to quantile regression for ecologists. Frontiers in Ecology and the Environment 1(8): 412-420. http://www.fort.usgs.gov/products/publications/21137/21137.pdf

Cizek, P. (2003): “Quantile Regression,” in XploRe Application Guide, ed. by W. Härdle, Z. Hlavka, and S. Klinke, chap. 1, pp. 19–48. Springer, Berlin.

Curry, J., and J. Gruber (1996): “Saving Babies: The Efficacy and Costs of Recent Changes in the Medicaid Eligibility of Pregnant Women,” Journal of Political Economy, 104, 457–470.

Handl, A. (2000): “Quantile,” available at http://www.wiwi.uni-bielefeld.de/~frohn/Lehre/Datenanalyse/Skript/daquantile.pdf

Härdle, W. (2003): Applied Multivariate Statistical Analysis. Springer Verlag, Heidelberg. Hyndman, R. J., and Y. Fan (1996): “Sample Quantiles in Statistical Packages,” The American Statistician, 50(4), 361 – 365.

Jeffreys, H., and B. S. Jeffreys (1988): Upper and Lower Bounds. Cambridge University Press.

Koenker, R., and G. W. Bassett (1978): “Regression Quantiles,” Econometrica, 46, 33–50.

Koenker, R., and G. W. Bassett (1982): “Robust tests for heteroscedasticity based on Regression Quantiles,” Econometrica, 61, 43–61.

Koenker, R., and K. F. Hallock (2000): “Quantile Regression an Introduction,” available at http://www.econ.uiuc.edu/~roger/research/intro/intro.html

Koenker, R., and K. F. Hallock (2001): “Quantile Regression,” Journal of Economic Perspectives, 15(4), 143–156.

Lee, S. (2005): “Lecture Notes for MECT1 Quantile Regression,” available at http://www.homepages.ucl.ac.uk/~uctplso/Teaching/MECT/lecture8.pdf

Lewit, E. M., L. S. Baker, H. Corman, and P. Shiono (1995): “The Direct Costs of Low Birth Weight,” The Future of Children, 5, 35–51.

mdbase (2005): “Statistical Methodology and Interactive Datanalysis,” available at http://www.quantlet.org/mdbase/

Montenegro, C. E. (2001): “Wage Distribution in Chile: Does Gender Matter? A Quantile Regression Approach,” Working Paper Series 20, The World Bank, Development Research Group.

Powell, J. (1986): “Censored Regression Quantiles,” Journal of Econometrics, 32, 143– 155.

Scharf, F. S., F. Juanes, and M. Sutherland (1998): “Inferring Ecologiocal Relationships from the Edges of Scatter Diagrams: Comparison of Regression Techniques,” Ecology, 79(2), 448–460.

XploRe (2006): “XploRe,” available at http://www.xplore-stat.de/index_js.html

# Numerical Comparison of Statistical Software

## Introduction

Statistical computations require an extra accuracy and are open to some errors such as truncation or cancellation error etc. These errors occur as a result of binary representation and finite precision and may cause inaccurate results. In this work we are going to discuss the accuracy of the statistical software, different tests and methods available for measuring the accuracy and the comparison of different packages.

### Accuracy of Software

Accuracy can be defined as the correctness of the results. When a statistical software package is used, it is assumed that the results are correct in order to comment on these results. On the other hand it must be accepted that computers have some limitations. The main problem is that the available precision provided by computer systems is limited. It is clear that statistical software can not deliver such accurate results, which exceed these limitations. However statistical software should recognize its limits and give clear indication that these limits are reached. We have two types of precision generally used today:

• Single precision
• Double precision

#### Binary Representation and Finite Precision

As we discussed above under the problem of software accuracy lay the binary representation and finite precision. In computer we don’t have real numbers. But we represent them with a finite approximation.

Example: Assume that we want to represent 0.1 in single precision. The result will be as follows:

0.1 = .00011001100110011001100110 = 0.99999964 (McCullough,1998)

It is clear that we can only approximate to 0.1 in binary form. This problem grows, if we try to subtract two large numbers which differs only in the decimals. For instance 100000.1-100000 = .09375

With single precision we can only represent 24 significant binary digits, with other word 6-7 decimal digits. In double precision it is possible to represent 53 significant binary digits and 15-17 significant decimal digits. Limitations of binary representation create five distinct numerical ranges, which cause the loss of accuracy:

• negative overflow
• negative underflow
• zero
• positive underflow
• positive overflow

Overflow means that values have grown too large for the representation. Underflow means that values are so small and so close to zero that causes to set to zero. Single and double precision representations have different ranges.

#### Results of Binary Representation

This limitations cause different errors in different situations:

• Cancellation error results from subtracting two nearly equal numbers.
• Accumulation errors are successive rounding errors in a series of calculations summed up to a total error. In this type of errors it is possible that only the rightmost digits of the result is affected or the result has no single accurate digits.
• Another result of binary representation and finite precision is that two formulas which are algebraically equivalent may not be equivalent numerically. For instance:
$\sum_{n=1}^{10000} n^{-2}$ $\sum_{n=1}^{10000} (10001-n)^{-2}$

First formula adds the numbers in ascending order, whereas the second in descending order. In the first formula the smallest numbers reached at the very end of the computation, so that these numbers are all lost to rounding error. The error is 650 times greater than the second.(McCullough,1998)

• Truncation error can be defined as approximation error which results from the limitations of binary representation.

Example:

$\sin x = x - \frac{x^3}{3!} + \frac{x^5}{5!} - \frac{x^7}{7!} + \cdots$

Difference between the true value of sin(x) and the result achieved by summing up finite number of terms is truncation error. (McCullough,1998)

• Algorithmic errors are another reason of inaccuracies. There can be different ways of calculating a quantity and these different methods may be unequally accurate. For example according to Sawitzki (1994) in a single precision environment using the following formula in order to calculate variance :
$S^2 = (1/(1-n)(\sum x_i^2 - n \bar x^2))$

### Measuring Accuracy

Due to limits of the computers some problems occur in calculating statistical values. We need a measure which shows us the degree of accuracy of a computed value. This measurement base on the difference between the computed value (q) and the real value (c).An oft-used measure is LRE (number of the correct significant digits)(McCullough,1998)

$LRE = -\log_{10} {\left[ |q-c|/|c| \right]}$

Rules:

• q should be close to c (less than 2). If they are not, set LRE to zero
• If LRE is greater than number of the digits in c, set LRE to number of the digits in c.
• If LRE is less than unity, set it to zero.

## Testing Statistical Software

In this part we are going to discuss two different tests which aim for measuring the accuracy of the software: Wilkinson Test (Wilkinson, 1985) and NIST StRD Benchmarks.

### Wilkinson's Statistic Quiz

Wilkinson dataset “NASTY” which is employed in Wilkinson’s Statistic Quiz is a dataset created by Leland Wilkinson (1985). This dataset consist of different variables such as “Zero” which contains only zeros, “Miss” with all missing values, etc. NASTY is a reasonable dataset in the sense of values it contains. For instance the values of “Big” in “NASTY” are less than U.S. Population or “Tiny” is comparable to many values in engineering. On the other hand the exercises of the “Statistic Quiz” are not meant to be reasonable. These tests are designed to check some specific problems in statistical computing. Wilkinson’s Statistics Quiz is an entry level test.

### NIST StRD Benchmarks

These benchmarks consist of different datasets designed by National Institute of Standards and Technology in different levels of difficulty. The purpose is to test the accuracy of statistical software regarding to different topics in statistics and different level of difficulty. In the webpage of “Statistical Reference Datasets” Project there are five groups of datasets:

• Analysis of Variance
• Linear Regression
• Markov Chain Monte Carlo
• Nonlinear Regression
• Univariate Summary Statistics

In all groups of benchmarks there are three different types of datasets: Lower level difficulty datasets, average level difficulty datasets and higher level difficulty datasets. By using these datasets we are going to explore whether the statistical software deliver accurate results to 15 digits for some statistical computations.

There are 11 datasets provided by NIST among which there are six datasets with lower level difficulty, two datasets with average level difficulty and one with higher level difficulty. Certified values to 15 digits for each dataset are provided for the mean (μ), the standard deviation (σ), the first-order autocorrelation coefficient (ρ).

In group of ANOVA-datasets there are 11 datasets with levels of difficulty, four lower, four average and three higher. For each dataset certified values to 15 digits are provided for between treatment degrees of freedom, within treatment. degrees of freedom, sums of squares, mean squares, the F-statistic , the R2, the residual standard deviation. Since most of the certified values are used in calculating the F-statistic, only its LRE λF will be compared to the result of regarding statistical software.

For testing the linear regression results of statistical software NIST provides 11 datasets with levels of difficulty two lower, two average and seven higher. For each dataset we have the certified values to 15 digits for coefficient estimates, standard errors of coefficients, the residual standard deviation, R2, the analysis of variance for linear regression table, which includes the residual sum of squares. LREs for the least accurate coefficients λβ, standard errors λσ and Residual sum of squares λr will be compared. In nonliner regression dataset group there are 27 datasets designed by NIST with difficulty eight lower ,eleven average and eight higher. For each dataset we have certified values to 11 digits provided by NIST for coefficient estimates, standard errors of coefficients, the residual sum of squares, the residual standard deviation, the degrees of freedom.

In the case of calculation of nonlinear regression we apply curve fitting method. In this method we need starting values in order to initialize each variable in the equation. Then we generate the curve and calculate the convergence criterion (ex. sum of squares). Then we adjust the variables to make the curve closer to the data points. There are several algorithms for adjusting the variables:

• The method of Marquardt and Levenberg
• The method of linear descent
• The method of Gauss-Newton

One of these methods is applied repeatedly, until the difference in the convergence criterion is smaller than the convergence tolerance.

NIST provides also two sets of starting values: Start I (values far from solution), Start II (values close to solution). Having Start II as initial values makes it easier to reach an accurate solution. Therefore Start I solutions will be preffered.

Other important settings are as follows:

• the convergence tolerance (ex. 1E-6)
• the method of solution (ex. Gauss Newton or Levenberg Marquardt)
• the convergence criterion (ex. residual sum of squares (RSS) or square of the maximum of the parameter differences)

We can also choose between numerical and analytic derivatives.

## Testing Examples

### Testing Software Package: SAS, SPSS and S-Plus

In this part we are going to discuss the test results of three statistical software packages applied by M.D. McCullough. In McCullough’s work SAS 6.12, SPSS 7.5 and S-Plus 4.0 are tested and compared in respect to certified LRE values provided by NIST. Comparison will be handled according to the following parts:

• Univariate Statistics
• ANOVA
• Linear Regression
• Nonlinear Regression

#### Univariate Statistics

Table 1: Results from SAS for Univariate Statistics (McCullough,1998)

All values calculated in SAS seem to be more or less accurate. For the dataset NumAcc1 p-value can not be calculated because of the insufficient number of observations. Calculating standard deviation for datasets NumAcc3 (average difficulty) and NumAcc 4 (high difficulty) seem to stress SAS.

Table 2: Results from SPSS for Univariate Statistics (McCullough,1998)

All values calculated for mean and standard deviation seem to be more or less accurate. For the dataset NumAcc1 p-value can not be calculated because of the insufficient number of observations.Calculating standard deviation for datasets NumAcc3 and -4 seem to stress SPSS,as well. For p-values SPSS represent results with only 3 decimal digits which causes an understate of first and an overstate of last p-values regarding to accuracy.

Table 3: Results from S-Plus for Univariate Statistics (McCullough,1998)

All values calculated for mean and standard deviation seem to be more or less accurate. S-Plus have also problems in calculating standard deviation for datasets NumAcc3 and -4. S-Plus does not show a good performance in calculating the p-values.

#### Analysis of Variance

Table 4: Results from SAS for Analysis of Variance(McCullough,1998)

Results:

• SAS can solve only the ANOVA problems of lower level difficulty.
• F-Statistics for datasets of average or higher difficulty can be calculated with very poor performance and zero digit accuracy.
• SPSS can display accurate results for datasets with lower level difficulty, like SAS.
• Performance of SPSS in calculating ANOVA is poor.
• For dataset “AtmWtAg” SPSS displays no F-Statistic which seems more logical instead of displaying zero accurate results.
• S-Plus handels ANOVA problem better than other softwares.
• Even for higher difficulty datasets this package can display more accurate results than other. But still results for datasets with high difficulty are not enough accurate.
• S-Plus can solve the average difficulty problems with a sufficient accuracy.

#### Linear Regression

Table 5: Results from SAS for Linear Regression(McCullough,1998)

SAS delivers no solution for dataset Filip which is ten degree polynomial. Except Filip SAS can display more or less accurate results. But the performance seems to decrease for higher difficulty datasets, especially in calculating coefficients

Table 6: Results from SPSS for Linear Regression(McCullough,1998)

SPSS has also Problems with “Filip” which is a 10 degree polynomial. Many packages fail to compute values for it. Like SAS, SPSS delivers lower accuracy for high level datasets

Table 7: Results from S-Plus for Linear Regression(McCullough,1998)

S-Plus is the only package which delivers a result for dataset “Filip”. The accuracy of Result for Filip seem not to be poor but average. Even for higher difficulty datasets S-Plus can calculate more accurate results than other software packages. Only coefficients for datasets “Wrampler4” and “-5” is under the average accuracy.

#### Nonlinear Regression

Table 8: Results from SAS for Nonlinear Regression(McCullough,1998)

For the nonlinear Regression two setting combinations are tested for each software, because different settings make a difference in the results.As we can see in the table in SAS preffered combination produce better results than default combination. In this table results produced using default combination are in paranthesis. Because 11 digits are provided for certified values by NIST, we are looking for LRE values of 11.

Preffered combination :

• Method:Gauss-Newton
• Criterion: PARAM
• Tolerance: 1E-6
Table 9: Results from SPSS for Nonlinear Regression(McCullough,1998)

Also in SPSS preffered combination shows a better performance than default options. All problems are solved with initial values “start I” whereas in SAS higher level datasets are solved with Start II values.

Preffered Combination:

• Method:Levenberg-Marquardt
• Criterion:PARAM
• Tolerance: 1E-12
Table 10: Results from S-Plus for Nonlinear Regression(McCullough,1998)

As we can see in the table preffered combination is also in S-Plus better than default combination. All problems except “MGH10” are solved with initial values “start I”. We may say that S-Plus showed a better performance than other software in calculating nonlinear regression.

Preffered Combination:

• Method:Gauss-Newton
• Tolerance: 1E-6

#### Results of the Comparison

All packages delivered accurate results for mean and standard deviation in univariate statistics.There are no big differences between the tested statistical software packages. In ANOVA calculations SAS and SPSS can not pass the average difficulty problems, whereas S-Plus delivered more accurate results than others. But for high difficulty datasets it also produced poor results. Regarding linear regression problems all packages seem to be reliable. If we examine the results for all software packages, we can say that the success in calculating the results for nonlinear regression greatly depends on the chosen options.

Other important results are as follows:

• S-Plus solved from Start II one time.
• SPSS never used Start II as initial values, but produce one time zero accurate digits.
• SAS used Start II three times and produced three times zero accurate digits.

### Comparison of different versions of SPSS

In this part we are going to compare an old version with a new version of SPSS in order to see whether the problems in older version are solved in the new one. In this part we compared SPSS version 7.5 with SPSS version 12.0. LRE values for version 7.5 are taken from an article by B.D. McCullough (see references). We also applied these tests to version 12.0 and calculated regarding LRE values. We chose one dataset from each difficulty groups and applied univariate statistics, ANOVA and linear regression in version 12.0. Source for the datasets is NIST Statistical Reference Datasets Archive. Then we computed LRE values for each dataset by using the certified values provided by NIST in order to compare two versions of SPSS.

#### Univariate Statistics

Difficulty: Low

Our first dataset is PiDigits with lower level difficulty which is designed by NIST in order to detect the deficiencies in calculating univariate statistical values.

Certified Values for PiDigits are as follows:

• Sample Mean : 4.53480000000000
• Sample Standard Deviation : 2.86733906028871
Table 11: Results from SPSS version 12.0 for dataset PiDigits

As we can see in the table 13 the results from SPSS 12.0 match the certified values provided by NIST. Therefore our LREs for mean and standard deviation are λμ: 15, λδ: 15. In version 7.5 LRE values were λμ: 14.7, λδ: 15. (McCullough,1998)

Difficulty: Average

Second dataset is NumAcc3 with average difficulty from NIST datasets for univariate statistics. Certified Values for NumAcc3 are as follows:

• Sample Mean : 1000000.2
• Sample Standard Deviation : 0.1
Table 12: Results from SPSS version 12.0 for dataset NumAcc3

In the table 14 we can see that calculated mean value is the same with the certified value by NIST. Therefore our LREs for mean is λμ: 15. However the standard deviation value differs from the certified value. So the calculation of LRE for standard deviation is as follows:

λδ : -log10 |0,10000000003464-0,1|/|0,1| = 9.5

LREs for SPSS v 7.5 were λμ: 15, λδ: 9.5. (McCullough,1998)

Difficulty: High

Last dataset in univariate statistics is NumAcc4 with high level of difficulty. Certified Values for NumAcc4 are as follows:

• Sample Mean : 10000000.2
• Sample Standard Deviation : 0.1
Table 13: Results from SPSS version 12.0 for dataset NumAcc4

Also for this dataset we do not have any problems with computed mean value. Therefore LRE is λμ: 15. However the standard deviation value does not match to the certified one. So we should calculate the LRE for standard deviation as follows:

λδ : -log10 |0,10000000056078-0,1|/|0,1| = 8.3

LREs for SPSS v 7.5 were λμ: 15, λδ : 8.3 (McCullough,1998)

For this part of our test we can say that there is no difference between two versions of SPSS. For average and high difficulty datasets delivered standard deviation results have still an average accuracy.

#### Analysis of Variance

Difficulty: Low

The dataset which we used for testing SPSS 12.0 regarding lower difficulty level problems is SiRstv. Certified F Statistic for SiRstv is 1.18046237440255E+00

Table 14: Results from SPSS version 12.0 for dataset SiRstv
• LRE : λF: -log10 | 1,18046237440224- 1,18046237440255|/ |1,18046237440255| = 12,58
• LRE for SPSS v 7.5 : λF : 9,6 (McCullough, 1998)

Difficulty: Average

Our dataset for average difficulty problems is AtmWtAg . Certified F statistic value for AtmWtAg is 1.59467335677930E+01.

File:Version12awa.jpg
Table 15: Results from SPSS version 12.0 for dataset AtmWtAg
• LREs : λF : -log10 | 15,9467336134506- 15,9467335677930|/| 15,9467335677930| = 8,5
• LREs for SPSS v 7.5 : λF: miss

Difficulty: High

We used the dataset SmnLsg07 in order to test high level difficulty problems. Certified F value for SmnLsg07 is 2.10000000000000E+01

Table 16: Results from SPSS version 12.0 for dataset SmnLsg07
• LREs : λF : -log10 | 21,0381922055595 - 21|/| 21| = 2,7
• LREs for SPSS v 7.5 : λF: 0

ANOVA results computed in version 12.0 are better than those calculated in version 7.5. However the accuracy degrees are still too low.

#### Linear Regression

Difficulty: Low

Our lower level difficulty dataset is Norris for linear regression. Certified values for Norris are as follows:

• Sample Residual Sum of Squares  : 26.6173985294224
• Table 17: Coefficient estimates for Norris(www.itl.nist.gov)
• LREs : λr : 9,9 λβ : 12,3 λσ : 10,2
• LREs for SPSS v 7.5 : λr: 9,9 , λβ : 12,3 , λσ : 10,2 (McCullough, 1998)
Table 18: Results from SPSS version 12.0 for dataset Norris

Difficulty: Average

We used the dataset NoInt1 in order to test the performance in average difficulty dataset. Regression model is as follows:

y = B1*x + e

Certified Values for NoInt1 :

• Sample Residual Sum of Squares  : 127,272727272727
• Coefficient estimate : 2.07438016528926, standard deviation : 0.16528925619834E-0(www.itl.nist.gov)
• LREs: λr:12,8 λβ: 15 λσ: 12,9
• LREs for SPSS v. 7.5 : λr: 12,8 , λβ: 14,7 , λσ: 12,5 (McCullough, 1998)
Table 19: Results from SPSS version 12.0 for dataset NoInt1

Difficulty: High

Our high level difficulty dataset is Longley designed by NIST.

• Model: y =B0+B1*x1 + B2*x2 + B3*x3 + B4*x4 + B5*x5 + B6*x6 +e
• LREs :
• λr: -log10 |836424,055505842-836424,055505915|/ |836424,055505915| = 13,1
• λβ : 15
• λσ : -log10 | 0,16528925619836E-01 – 0,16528925619834E-01|/ |0,16528925619834E-01| = 12,9
• LREs for SPSS v. 7.5 : λr: 12,8 , λβ : 14,7 , λσ : 12,5 (McCullough, 1998)

As we conclude from the computed LREs, there is no big difference between the results of two versions for linear regression.

## Conclusion

By applying these test we try to find out whether the software are reliable and deliver accurate results or not. However based on the results we can say that different software packages deliver different results for same the problem which can lead us to wrong interpretations for statistical research questions.

In specific we can that SAS, SPSS and S-Plus can solve the linear regression problems better in comparision to ANOVA Problems. All three of them deliver poor results for F statistic calculation.

From the results of comparison two different versions of SPSS we can conclude that the difference between the accuracy of the results delivered by SPSS v.12 and v.7.5 is not great considering the difference between the version numbers. On the other hand SPSS v.12 can handle the ANOVA Problems much better than old version. However it has still problems in higher difficulty problems.

## References

• McCullough, B.D. 1998, 'Assessing The Reliability of Ststistical Software: Part I',The American Statistician, Vol.52, No.4, pp.358-366.
• McCullough, B.D. 1999, 'Assessing The Reliability of Ststistical Software: Part II', The American Statistician, Vol.53, No.2, pp.149-159
• Sawitzki, G. 1994, 'Testing Numerical Reliability of Data Analysis Systems', Computational Statistics & Data Analysis, Vol.18, No.2, pp.269-286
• Wilkinson, L. 1993, 'Practical Guidelines for Testing Statistical Software' in 25th Conference on Statistical Computing at Schloss Reisenburg, ed. P. Dirschedl& R. Ostermnann, Physica Verlag
• National Institute of Standards and Technology. (1 September 2000). The Statistical Reference Datasets: Archives, [Online], Available from: <http://www.itl.nist.gov/div898/strd/general/dataarchive.html> [10 November 2005].

# Numerics in Excel

The purpose of this paper is to evaluate the accuracy of MS Excel in terms of statistical procedures and to conclude whether the MS Excel should be used for (statistical) scientific purposes or not. The evaulation is made for Excel versions 97, 2000, XP and 2003.

According to the literature, there are three main problematic areas for Excel if it is used for statistical calculations. These are

• probability distributions,
• univariate statistics, ANOVA and Estimations (both linear and non-linear)
• random number generation.

If the results of statistical packages are assessed, one should take into account that the acceptable accuracy of the results should be achieved in double precision (which means that a result is accepted as accurate if it possesses 15 accurate digits) given that the reliable algorithms are capable of delivering correct results in double precision, as well. If the reliable algorithms can not retrieve results in double precision, it is not fair to anticipate that the package (evaluated) should achieve double precision. Thus we can say that the correct way for evaluating the statistical packages is assessing the quality of underlying algorithm of statistical calculations rather than only counting the accurate digits of results. Besides, test problems must be reasonable which means they must be amenable to solution by known reliable algorithms. (McCullough & Wilson, 1999, S. 28)

In further sections, our judgement about the accuracy of MS Excel will base on certified values and tests. As basis we have Knüsel’s ELV software for probability distributions, StRD (Statistical Reference Datasets) for Univariate Statistics, ANOVA and Estimations and finally Marsaglia’s DIEHARD for Random Number Generation. Each of the tests and certified values will be explained in the corresponding sections.

## Assessing Excel Results for Statistical Distributions

As we mentioned above our judgement about Excel’s calculations for probability distributions will base on Knüsel’s ELV Program which can compute probabilities and quantiles of some elementary statistical distributions. Using ELV, the upper and lower tail probabilities of all distributions are computed with six significant digits for probabilities as small as 10−100 and upper and lower quantiles are computed for all distributions for tail probabilities P with 10−12 ≤ P ≤ ½. (Knüsel, 2003, S.1)

In our benchmark Excel should display no inaccurate digits. If six digits are displayed, then all six digits should be correct. If the algorithm is only accurate to two digits, then only two digits should be displayed so as not to mislead the user (McCullough & Wilson, 2005, S. 1245)

In the following sub-sections the exact values in the tables are retrieved from Knüsel’s ELV software and the acceptable accuracy is in single presicion, because even the best algorithms can not achieve 15 correct digits in most cases, if the probability distributions are issued.

### Normal Distribution

• Excel Function:NORMDIST
• Parameters: mean = 0, variance = 1, x (critical value)
• Computes: the tail probability Pr X ≤ x, whereas X denotes a random variable with a standard normal distribution (with mean 0 and variance 1)
Table 1: (Knüsel, 1998, S.376)

As we can see in table 1, Excel 97, 2000 and XP encounter problems and computes small probabilities in tail incorrectly (i.e for x = -8,3 or x = -8.2) However, this problem is fixed in Excel 2003 (Knüsel, 2005, S.446).

### Inverse Normal Distribution

• Excel Function: NORMINV
• Parameters: mean = 0, variance = 1, p (probability for X < x)
• Computes: the x value (quantile)

X denotes a random variable with a standard normal distribution. In contrast to “NORMDIST” function issued in the last section, p is given and quantile is computed.

If used, Excel 97 prints out quantiles with 10 digits although none of these 10 digits may be correct if p is small. In Excel 2000 and XP, Microsoft tried to fix errors, although results are not sufficient (See table 2). However in Excel 2003 the problem is fixed entirely. (Knüsel, 2005, S.446)

Table 2: (Knüsel, 2002, S.110)

### Inverse Chi-Square Distribution

• Excel Function: CHIINV
• Parameters: p (probability for X > x), n (degrees of freedom)
• Computes: the x value (quantile)

X denotes a random variable with a chi-square distribution with n degrees of freedom.

Table 3: (Knüsel , 1998, S. 376)

Old Excel Versions: Although the old Excel versions show ten significant digits, only very few of them are accurate if p is small (See table 3). Even if p is not small, the accurate digits are not enough to say that Excel is sufficient for this distribution.

Excel 2003: Problem was fixed. (Knüsel, 2005, S.446)

### Inverse F Distribution

• Excel Function: FINV
• Parameters: p (probability for X > x), n1, n2 (degrees of freedom)
• Computes: the x value (quantile)

X denotes a random variable with a F distribution with n1 and n2 degrees of freedom.

Table 4: (Knüsel , 1998, S. 377)

Old Excel Versions: Excel prints out x values with 7 or more significant digits although only one or two of these many digits are correct if p is small (See table 4).

Excel 2003: Problem fixed. (Knüsel, 2005, S.446)

### Inverse t Distribution

• Excel Function: TINV
• Parameters: p (probability for |X| > x), n (degree of freedom)
• Computes: the x value (quantile)

X denotes a random variable with a t distribution with n degrees of freedom. Please note that the |X| value causes a 2 tailed computation. (lower tail & high tail)

Table 5: (Knüsel , 1998, S. 377)

Old Excel Versions: Excel prints out quantiles with 9 or more significant digits although only one or two of these many digits are correct if p is small (See table 5).

Excel 2003: Problem fixed. (Knüsel, 2005, S.446)

### Poisson Distribution

• Excel Function: Poisson
• Parameters: λ (mean), k (number of cases)
• Computes: the tail probability Pr X ≤ k

X denotes a random variable with a Poisson distribution with given parameters.

Table 6: (McCullough & Wilson, 2005, S.1246)

Old Excel Versions: correctly computes very small probabilities but gives no result for central probabilities near the mean (in the range about 0.5). (See table 6)

Excel 2003: The central probabilities are fixed. However, inaccurate results in the tail. (See table 6)

The strange behaivour of Excel can be encountered for values λ150. (Knüsel, 1998, S.375) It fails even for probabilities in the central range between 0.01 and 0.99 and even for parameter values that cannot be judged as too extreme.

### Binomial Distribution

• Excel Function: BINOMDIST
• Parameters: n (= number of trials) , υ(= probability for a success) , k(number of successes)
• Computes: the tail probability Pr X ≤ k

-X denotes a random variable with a binoamial distribution with given parameters

Table 7: (Knüsel, 1998, S.375)

Old Excel Versions: As we see in table 7, old versions of Excel correctly computes very small probabilities but gives no result for central probabilities near the mean (same problem with Poisson distribuiton on old Excel versions)

Excel 2003: The central probabilities are fixed. However, inaccurate results in the tail. (Knüsel, 2005, S.446). (same problem with Poisson distribuiton on Excel 2003).

This strange behaivour of Excel can be encountered for values n > 1000. (Knüsel, 1998, S.375) It fails even for probabilities in the central range between 0.01 and 0.99 and even for parameter values that cannot be judged as too extreme.

### Other problems

• Excel 97, 2000 and XP includes flaws by computing the hypergeometric distribution (HYPERGEOM). For some values (N > 1030) no result is retrieved. This is prevented on Excel 2003, but there is still no option to compute tail probabilities. So computation of Pr {X = k} is possible, but computation of Pr {X ≤ k} is not. (Knüsel, 2005, S.447)
• Function GAMMADIST for gamma distribution retreives incorrect values on Excel 2003. (Knüsel, 2005, S.447-448)
• Also the function BETAINV for inverse beta distribution computes incorrect values on Excel 2003 (Knüsel, 2005, S. 448)

## Assessing Excel Results for Univariate Statistics, ANOVA and Estimation (Linear & Non-Linear)

Our judgement about Excel’s calculations for univariate statistics, ANOVA and Estimation will base on StRD which is designed by Statistical Engineering Division of National Institute of Standards and Technology (NIST) to assist researchers in benchmarking statistical software packages explicitly. StRD has reference datasets (real-world and generated datasets) with certified computational results that enable the objective evaluation of statistical Software. It comprises four suites of numerical benchmarks for statistical software: univariate summary statistics, one way analysis of variance, linear regression and nonlinear regression and it includes several problems for each suite of tests. All problems have a difficulty level:low, average or high.

By assessing Excel results in this section we are going to use LRE (log relative error) which can be used as a score for accuracy of results of statistical packages. The number of correct digits in results can be calculated via log relative error. Please note that for double precision the computed LRE is in the range 0 - 15, because we can have max. 15 correct digits in double precision.

Formula LRE:

$\lambda = LRE(x) = -log_{10} \left ( \frac{|x - c|}{|x|} \right )$

c: the correct answer (certified computational result) for a particular test problem

x: answer of Excel for the same problem

### Univariate Statistics

• Excel Functions: - AVERAGE, STDEV, PEARSON (also CORREL)
• Computes (respectively): mean, standard deviation, correlation coefficient
Table 8: (McCullough & Wilson, 2005, S.1247)

Old Excel Versions: an unstable algorithm for calculation of the sample variance and the correlation coefficient is used. Even for the low difficulty problems (datasets with letter “l” in table 8) the old versions of Excel fail.

Excel 2003: Problem was fixed and the performance is acceptable. The accurate digits less than 15 don’t indicate an unsuccessful implementation because even the reliable algorithms can not retrieve 15 correct digits for these average and high difficulty problems (datasets with letters “a” and “h” in table 8) of StRD.

### ONEWAY ANOVA

• Excel Function: Tools – Data Analysis – ANOVA: Single Factor (requires Analysis Toolpak)
• Computes: df, ss, ms, F-statistic

Since ANOVA produces many numerical results (such as df, ss, ms, F), here only the LRE for the final F-statistic is presented. Before assessing Excel’s performance one should consider that a reliable algorithm for one way Analysis of Variance can deliver 8-10 digits for the average difficulty problems and 4-5 digits for higher difficulty problems.

Table 9: (McCullough & Wilson, 2005, S.1248)

Old Excel Versions: Considering numerical solutions, delivering only a few digits of accuracy for difficult problems is not an evidence for bad software, but retrieving 0 accurate digits for average difficulty problems indicates bad software when calculating ANOVA. (McCullough & Wilson, 1999, S. 31). For that reason Excel versions prior than Excel 2003 has an acceptable performance only on low-difficulty problems. It retrieves zero accurate digits for difficult problems. Besides, negative results for “within group sum of squares” and “between group sum of squares” are the further indicators of a bad algorithm used for Excel. (See table 9)

Excel 2003: Problem was fixed (See table 9). The zero digits of accuracy for the Simon 9 test is no cause for concern, since this also occurs when reliable algorithms are employed. Therefore the performance is acceptable. (McCullough & Wilson, 2005, S. 1248)

### Linear Regression

• Excel Function: LINEST
• Computes: All numerical results required by Linear Regression

Since LINEST produces many numerical results for linear regression, only the LRE for the coefficients and standard errors of coefficients are taken into account. Table 9 shows the lowest LRE values for each dataset as the weakest link in the chain in order to reflect the worst estimations (smallest λβ-LRE and λσ-LRE) made by Excel for each linear regression function.

Old Excel Versions: either doesn't check for near-singularity of the input matrix or checking it incorrectly, so the results for ill-conditioned Dataset “Filip (h)” include not a single correct digit. Actually, Excel should have refused the solution and commit a warning to user about the near singularity of data matrix. (McCullough & Wilson, 1999, S.32,33) . However, in this case, the user is mislead.

Excel 2003: Problem is fixed and Excel 2003 has an acceptable performance. (see table 10)

Table 10: (McCullough & Wilson, 1999, S. 32)

### Non-Linear Regression

When solving nonlinear regression using Excel, it is possible to make choices about:

1. method of derivative calculation: forward (default) or central numerical derivatives
2. convergence tolerance (default=1.E-3)
3. scaling (recentering) the variables
4. method of solution (default – GRG2 quasi-Newton method)

Excel’s default parameters don’t always produce the best solutions always (like all other solvers). Therefore one needs to give different parameters and test the Excel-Solver for non-linear regression. In table 10 the columns A-B-C-D are combinations of different non-linear options. Because changing the 1st and 4th option doesn’t affect the result, only 2nd and 3rd parameters are changed for testing:

• A: Default estimation
• B: Convergence Tolerance = 1E -7
• C: Automatic Scaling
• D: Convergence Tolerance = 1E -7 & Automatic Scaling

In Table 11, the lowest LRE principle is applied to simplify the assessment. (like in linear reg.)

Results in table 11 are same for each Excel version (Excel 97, 2000, XP, 2003)

Table 11: (McCullough & Wilson, 1999, S. 34)

As we see in table 11, the non-linear option combination A produces 21 times, B 17 times, C 20 times and D 14 times “0” accurate digits. which indicates that the performance of Excel in this area is inadequate. Expecting to find all exact solutions for all problems with Excel is not fair, but if it is not able to find the result, it is expected to warn user and commit that the solution can not be calculated. Furthermore, one should emphasize that other statistical packages like SPSS, S-PLUS and SAS exhibit zero digit accuracy only few times (0 to 3) in these tests (McCullough & Wilson, 1999, S. 34).

## Assessing Random Number Generator of Excel

Many statistical procedures employ random numbers and it is expected that the generated random numbers are really random. Only random number generators should be used that have solid theoretical properties. Additionally, statistical tests should be applied on samples generated and only generators whose output has successfuly passed a battery of statistical tests should be used. (Gentle, 2003)

Based on the facts explained above we should assess the quality of Random Number Generation by:

• analysing the underlying algorithm for Random Number Generation.
• analysing the generators output stream. There are many alternatives to test the output of a RNG. One can evaluate the generated output using static tests in which the generation order is not important. These tests are goodness of fit tests. The second way of evaluating the output stream is running a dynamic test on generator, whereas the generation order of the numbers is important.

### Excel’s RNG – Underlying algorithm

The objective of random number generation is to produce samples any given size that are indistinguishable from samples of the same size from a U(0,1) distribution. (Gentle, 2003) For this purpose there are different algorithms to use. Excel’s algorithm for random number generation is Wichmann–Hill algorithm. Wichmann–Hill is a useful RNG algorithm for common applications, but it is obsolete for modern needs (McCullough & Wilson, 2005, S. 1250). The formula for this random number generator is defined as follows:

Xi = 171.Xi − 1mod30269

Yi = 172.Yi − 1mod30307

Zi = 170.Zi − 1mod30323

$U_i = \frac{X_i}{30269} + \frac{Y_i}{30307} + \frac {Z_i}{30323} mod 1$

Wichmann–Hill is a congruential generator which means that it is a recursive aritmethical RNG as we see in the formula above. It is a combination of three other linear congruential generator and requires three seeds: X0Y0Z 0.

Period, in terms of random number generation, is the number of calls that can be made to the RNG before it begins to repeat. For that reason, having a long period is a quality measure for random number generators. It is essential that the period of the generator be larger than the number of random numbers to be used. Modern applications are increasingly demanding longer and longer sequences of random numbers (i.e for using in Monte-Carlo simulations) (Gentle, 2003)

The lowest acceptable period for a good RNG is 260 and the period of Wichmann-Hill RNG is 6.95E+12 (≈ 243). In addition to this unacceptable performance, Microsoft claims that the period of Wichmann-Hill RNG is 10E+13 Even if Excel’s RNG has a period of 10E+13, it is still not sufficient to be an acceptable random number generator because this value is also less than 260. (McCullough & Wilson, 2005, S. 1250)

Furthermore it is known that RNG of Excel produces negative values after the RNG executed many times. However a correct implementation of a Wichmann-Hill Random Number Generator should produce only values between 0 and 1. (McCullough & Wilson, 2005, S. 1249)

### Excel’s RNG – The Output Stream

As we discussed above, it is not sufficient to discuss only the underlying algorithm of a random number generation. One needs also some tests on output stream of a random number generator while assessing the quality of this random number generator. So a Random Number Generator should produce output which passes some tests for randomness. Such a battery of tests, called DIEHARD, has been prepared by Marsaglia. A good RNG should pass almost all of the tests but as we can see in table 12 Excel can pass only 11 of them (7 failure), although Microsoft has declaired Wichmann–Hill Algorithm is implemented for Excel’s RNG. However, we know that Wichmann-Hill is able to pass 16 tests from DIEHARD (McCullough & Wilson, 1999, S. 35).

Due to reasons explained in previous and this section we can say that Excel’s performance is inadequate (because of period length, incorrect implementation Wichmann Hill Algorithm, which is already obsolete, DIEHARD test results)

Table 12: (McCullough & Wilson, 1999, S. 35)

## Conclusion

Old versions of Excel (Excel 97, 2000, XP) :

• shows poor performance on following distributions: Normal, F, t, Chi Square, Binomial, Poisson, Hypergeometric
• retrieves inadequate results on following calculations: Univariate statistics, ANOVA, linear regression, non-linear regression
• has an unacceptable random number generator

For those reasons, we can say that use of Excel 97, 2000, XP for (statistical) scientific purposes should be avoided.

Although several bugs are fixed in Excel 2003, still use of Excel for (statistical) scientific purposes should be avoided because it:

• has a poor performance on following distributions: Binomial, Poisson, Gamma, Beta
• retrieves inadequate results for non-linear regression
• has an obsolete random number generator.

## References

• Gentle J.E. (2003) Random number generation and Monte Carlo methods 2nd edition. New York Springer Verlag
• Knüsel, L. (2003) Computation of Statistical Distributions Documentation of the Program ELV Second Edition. http://www.stat.uni-muenchen.de/~knuesel/elv/elv_docu.pdf Retrieved [13 November 2005]
• Knüsel, L. (1998). On the Accuracy of the Statistical Distributions in Microsoft Excel 97. Computational Statistics and Data Analysis (CSDA), Vol. 26, 375-377.
• Knüsel, L. (2002). On the Reliability of Microsoft Excel XP for statistical purposes. Computational Statistics and Data Analysis (CSDA), Vol. 39, 109-110.
• Knüsel, L. (2005). On the Accuracy of Statistical Distributions in Microsoft Excel 2003. Computational Statistics and Data Analysis (CSDA), Vol. 48, 445-449.
• McCullough, B.D. & Wilson B. (2005). On the accuracy of statistical procedures in Microsoft Excel 2003. Computational Statistics & Data Analysis (CSDA), Vol. 49, 1244 – 1252.
• McCullough, B.D. & Wilson B. (1999). On the accuracy of statistical procedures in Microsoft Excel 97. Computational Statistics & Data Analysis (CSDA), Vol. 31, 27– 37.
• PC Magazin, April 6, 2004, p.71*

## Resources

Excel Statistics Lab Manual is written in Excel.

# Authors

Authors and contributors to this book include:

• Cronian
• Llywelyn
• Murraytodd
• Sigbert
• Urimeir
• Zginder

# Glossary

This is a glossary of the book.

MediaWiki:Toc: Top - 0–9 A B C D E F G H I J K L M N O P Q R S T U V W X Y Z

## P

primary data
Original data that have been collected specially for the purpose in mind.

## S

secondary data
Data that have been collected for another purpose and where we will use Statistical Method with the Primary Data.

Version 1.2, November 2002

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The purpose of this License is to make a manual, textbook, or other functional and useful document "free" in the sense of freedom: to assure everyone the effective freedom to copy and redistribute it, with or without modifying it, either commercially or noncommercially. Secondarily, this License preserves for the author and publisher a way to get credit for their work, while not being considered responsible for modifications made by others.

This License is a kind of "copyleft", which means that derivative works of the document must themselves be free in the same sense. It complements the GNU General Public License, which is a copyleft license designed for free software.

We have designed this License in order to use it for manuals for free software, because free software needs free documentation: a free program should come with manuals providing the same freedoms that the software does. But this License is not limited to software manuals; it can be used for any textual work, regardless of subject matter or whether it is published as a printed book. We recommend this License principally for works whose purpose is instruction or reference.

## 1. APPLICABILITY AND DEFINITIONS

This License applies to any manual or other work, in any medium, that contains a notice placed by the copyright holder saying it can be distributed under the terms of this License. Such a notice grants a world-wide, royalty-free license, unlimited in duration, to use that work under the conditions stated herein. The "Document", below, refers to any such manual or work. Any member of the public is a licensee, and is addressed as "you". You accept the license if you copy, modify or distribute the work in a way requiring permission under copyright law.

A "Modified Version" of the Document means any work containing the Document or a portion of it, either copied verbatim, or with modifications and/or translated into another language.

A "Secondary Section" is a named appendix or a front-matter section of the Document that deals exclusively with the relationship of the publishers or authors of the Document to the Document's overall subject (or to related matters) and contains nothing that could fall directly within that overall subject. (Thus, if the Document is in part a textbook of mathematics, a Secondary Section may not explain any mathematics.) The relationship could be a matter of historical connection with the subject or with related matters, or of legal, commercial, philosophical, ethical or political position regarding them.

The "Invariant Sections" are certain Secondary Sections whose titles are designated, as being those of Invariant Sections, in the notice that says that the Document is released under this License. If a section does not fit the above definition of Secondary then it is not allowed to be designated as Invariant. The Document may contain zero Invariant Sections. If the Document does not identify any Invariant Sections then there are none.

The "Cover Texts" are certain short passages of text that are listed, as Front-Cover Texts or Back-Cover Texts, in the notice that says that the Document is released under this License. A Front-Cover Text may be at most 5 words, and a Back-Cover Text may be at most 25 words.

A "Transparent" copy of the Document means a machine-readable copy, represented in a format whose specification is available to the general public, that is suitable for revising the document straightforwardly with generic text editors or (for images composed of pixels) generic paint programs or (for drawings) some widely available drawing editor, and that is suitable for input to text formatters or for automatic translation to a variety of formats suitable for input to text formatters. A copy made in an otherwise Transparent file format whose markup, or absence of markup, has been arranged to thwart or discourage subsequent modification by readers is not Transparent. An image format is not Transparent if used for any substantial amount of text. A copy that is not "Transparent" is called "Opaque".

Examples of suitable formats for Transparent copies include plain ASCII without markup, Texinfo input format, LaTeX input format, SGML or XML using a publicly available DTD, and standard-conforming simple HTML, PostScript or PDF designed for human modification. Examples of transparent image formats include PNG, XCF and JPG. Opaque formats include proprietary formats that can be read and edited only by proprietary word processors, SGML or XML for which the DTD and/or processing tools are not generally available, and the machine-generated HTML, PostScript or PDF produced by some word processors for output purposes only.

The "Title Page" means, for a printed book, the title page itself, plus such following pages as are needed to hold, legibly, the material this License requires to appear in the title page. For works in formats which do not have any title page as such, "Title Page" means the text near the most prominent appearance of the work's title, preceding the beginning of the body of the text.

A section "Entitled XYZ" means a named subunit of the Document whose title either is precisely XYZ or contains XYZ in parentheses following text that translates XYZ in another language. (Here XYZ stands for a specific section name mentioned below, such as "Acknowledgements", "Dedications", "Endorsements", or "History".) To "Preserve the Title" of such a section when you modify the Document means that it remains a section "Entitled XYZ" according to this definition.

The Document may include Warranty Disclaimers next to the notice which states that this License applies to the Document. These Warranty Disclaimers are considered to be included by reference in this License, but only as regards disclaiming warranties: any other implication that these Warranty Disclaimers may have is void and has no effect on the meaning of this License.

## 2. VERBATIM COPYING

You may copy and distribute the Document in any medium, either commercially or noncommercially, provided that this License, the copyright notices, and the license notice saying this License applies to the Document are reproduced in all copies, and that you add no other conditions whatsoever to those of this License. You may not use technical measures to obstruct or control the reading or further copying of the copies you make or distribute. However, you may accept compensation in exchange for copies. If you distribute a large enough number of copies you must also follow the conditions in section 3.

You may also lend copies, under the same conditions stated above, and you may publicly display copies.

## 3. COPYING IN QUANTITY

If you publish printed copies (or copies in media that commonly have printed covers) of the Document, numbering more than 100, and the Document's license notice requires Cover Texts, you must enclose the copies in covers that carry, clearly and legibly, all these Cover Texts: Front-Cover Texts on the front cover, and Back-Cover Texts on the back cover. Both covers must also clearly and legibly identify you as the publisher of these copies. The front cover must present the full title with all words of the title equally prominent and visible. You may add other material on the covers in addition. Copying with changes limited to the covers, as long as they preserve the title of the Document and satisfy these conditions, can be treated as verbatim copying in other respects.

If the required texts for either cover are too voluminous to fit legibly, you should put the first ones listed (as many as fit reasonably) on the actual cover, and continue the rest onto adjacent pages.

If you publish or distribute Opaque copies of the Document numbering more than 100, you must either include a machine-readable Transparent copy along with each Opaque copy, or state in or with each Opaque copy a computer-network location from which the general network-using public has access to download using public-standard network protocols a complete Transparent copy of the Document, free of added material. If you use the latter option, you must take reasonably prudent steps, when you begin distribution of Opaque copies in quantity, to ensure that this Transparent copy will remain thus accessible at the stated location until at least one year after the last time you distribute an Opaque copy (directly or through your agents or retailers) of that edition to the public.

It is requested, but not required, that you contact the authors of the Document well before redistributing any large number of copies, to give them a chance to provide you with an updated version of the Document.

## 4. MODIFICATIONS

You may copy and distribute a Modified Version of the Document under the conditions of sections 2 and 3 above, provided that you release the Modified Version under precisely this License, with the Modified Version filling the role of the Document, thus licensing distribution and modification of the Modified Version to whoever possesses a copy of it. In addition, you must do these things in the Modified Version:

A. Use in the Title Page (and on the covers, if any) a title distinct from that of the Document, and from those of previous versions (which should, if there were any, be listed in the History section of the Document). You may use the same title as a previous version if the original publisher of that version gives permission.
B. List on the Title Page, as authors, one or more persons or entities responsible for authorship of the modifications in the Modified Version, together with at least five of the principal authors of the Document (all of its principal authors, if it has fewer than five), unless they release you from this requirement.
C. State on the Title page the name of the publisher of the Modified Version, as the publisher.
D. Preserve all the copyright notices of the Document.
F. Include, immediately after the copyright notices, a license notice giving the public permission to use the Modified Version under the terms of this License, in the form shown in the Addendum below.
G. Preserve in that license notice the full lists of Invariant Sections and required Cover Texts given in the Document's license notice.
H. Include an unaltered copy of this License.
I. Preserve the section Entitled "History", Preserve its Title, and add to it an item stating at least the title, year, new authors, and publisher of the Modified Version as given on the Title Page. If there is no section Entitled "History" in the Document, create one stating the title, year, authors, and publisher of the Document as given on its Title Page, then add an item describing the Modified Version as stated in the previous sentence.
J. Preserve the network location, if any, given in the Document for public access to a Transparent copy of the Document, and likewise the network locations given in the Document for previous versions it was based on. These may be placed in the "History" section. You may omit a network location for a work that was published at least four years before the Document itself, or if the original publisher of the version it refers to gives permission.
K. For any section Entitled "Acknowledgements" or "Dedications", Preserve the Title of the section, and preserve in the section all the substance and tone of each of the contributor acknowledgements and/or dedications given therein.
L. Preserve all the Invariant Sections of the Document, unaltered in their text and in their titles. Section numbers or the equivalent are not considered part of the section titles.
M. Delete any section Entitled "Endorsements". Such a section may not be included in the Modified Version.
N. Do not retitle any existing section to be Entitled "Endorsements" or to conflict in title with any Invariant Section.
O. Preserve any Warranty Disclaimers.

If the Modified Version includes new front-matter sections or appendices that qualify as Secondary Sections and contain no material copied from the Document, you may at your option designate some or all of these sections as invariant. To do this, add their titles to the list of Invariant Sections in the Modified Version's license notice. These titles must be distinct from any other section titles.

You may add a section Entitled "Endorsements", provided it contains nothing but endorsements of your Modified Version by various parties--for example, statements of peer review or that the text has been approved by an organization as the authoritative definition of a standard.

You may add a passage of up to five words as a Front-Cover Text, and a passage of up to 25 words as a Back-Cover Text, to the end of the list of Cover Texts in the Modified Version. Only one passage of Front-Cover Text and one of Back-Cover Text may be added by (or through arrangements made by) any one entity. If the Document already includes a cover text for the same cover, previously added by you or by arrangement made by the same entity you are acting on behalf of, you may not add another; but you may replace the old one, on explicit permission from the previous publisher that added the old one.

The author(s) and publisher(s) of the Document do not by this License give permission to use their names for publicity for or to assert or imply endorsement of any Modified Version.

## 5. COMBINING DOCUMENTS

You may combine the Document with other documents released under this License, under the terms defined in section 4 above for modified versions, provided that you include in the combination all of the Invariant Sections of all of the original documents, unmodified, and list them all as Invariant Sections of your combined work in its license notice, and that you preserve all their Warranty Disclaimers.

The combined work need only contain one copy of this License, and multiple identical Invariant Sections may be replaced with a single copy. If there are multiple Invariant Sections with the same name but different contents, make the title of each such section unique by adding at the end of it, in parentheses, the name of the original author or publisher of that section if known, or else a unique number. Make the same adjustment to the section titles in the list of Invariant Sections in the license notice of the combined work.

In the combination, you must combine any sections Entitled "History" in the various original documents, forming one section Entitled "History"; likewise combine any sections Entitled "Acknowledgements", and any sections Entitled "Dedications". You must delete all sections Entitled "Endorsements."

## 6. COLLECTIONS OF DOCUMENTS

You may make a collection consisting of the Document and other documents released under this License, and replace the individual copies of this License in the various documents with a single copy that is included in the collection, provided that you follow the rules of this License for verbatim copying of each of the documents in all other respects.

You may extract a single document from such a collection, and distribute it individually under this License, provided you insert a copy of this License into the extracted document, and follow this License in all other respects regarding verbatim copying of that document.

## 7. AGGREGATION WITH INDEPENDENT WORKS

A compilation of the Document or its derivatives with other separate and independent documents or works, in or on a volume of a storage or distribution medium, is called an "aggregate" if the copyright resulting from the compilation is not used to limit the legal rights of the compilation's users beyond what the individual works permit. When the Document is included in an aggregate, this License does not apply to the other works in the aggregate which are not themselves derivative works of the Document.

If the Cover Text requirement of section 3 is applicable to these copies of the Document, then if the Document is less than one half of the entire aggregate, the Document's Cover Texts may be placed on covers that bracket the Document within the aggregate, or the electronic equivalent of covers if the Document is in electronic form. Otherwise they must appear on printed covers that bracket the whole aggregate.

## 8. TRANSLATION

Translation is considered a kind of modification, so you may distribute translations of the Document under the terms of section 4. Replacing Invariant Sections with translations requires special permission from their copyright holders, but you may include translations of some or all Invariant Sections in addition to the original versions of these Invariant Sections. You may include a translation of this License, and all the license notices in the Document, and any Warranty Disclaimers, provided that you also include the original English version of this License and the original versions of those notices and disclaimers. In case of a disagreement between the translation and the original version of this License or a notice or disclaimer, the original version will prevail.

If a section in the Document is Entitled "Acknowledgements", "Dedications", or "History", the requirement (section 4) to Preserve its Title (section 1) will typically require changing the actual title.

## 9. TERMINATION

You may not copy, modify, sublicense, or distribute the Document except as expressly provided for under this License. Any other attempt to copy, modify, sublicense or distribute the Document is void, and will automatically terminate your rights under this License. However, parties who have received copies, or rights, from you under this License will not have their licenses terminated so long as such parties remain in full compliance.

## 10. FUTURE REVISIONS OF THIS LICENSE

The Free Software Foundation may publish new, revised versions of the GNU Free Documentation License from time to time. Such new versions will be similar in spirit to the present version, but may differ in detail to address new problems or concerns. See http://www.gnu.org/copyleft/.

Each version of the License is given a distinguishing version number. If the Document specifies that a particular numbered version of this License "or any later version" applies to it, you have the option of following the terms and conditions either of that specified version or of any later version that has been published (not as a draft) by the Free Software Foundation. If the Document does not specify a version number of this License, you may choose any version ever published (not as a draft) by the Free Software Foundation.