# Errors and residuals in statistics

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In statistics and optimization, **statistical errors** and **residuals** are two closely related and easily confused measures of the deviation of an observed value of an element of a statistical sample from its "theoretical value". The **error** (or **disturbance**) of an observed value is the deviation of the observed value from the (unobservable) *true* function value, while the **residual** of an observed value is the difference between the observed value and the *estimated* function value.

The distinction is most important in regression analysis, where it leads to the concept of studentized residuals.

## Contents

## Introduction

Suppose there is a series of observations from a univariate distribution and we want to estimate the mean of that distribution (the so-called location model). In this case, the errors are the deviations of the observations from the population mean, while the residuals are the deviations of the observations from the sample mean.

A **statistical error** (or **disturbance**) is the amount by which an observation differs from its expected value, the latter being based on the whole population from which the statistical unit was chosen randomly. For example, if the mean height in a population of 21-year-old men is 1.75 meters, and one randomly chosen man is 1.80 meters tall, then the "error" is 0.05 meters; if the randomly chosen man is 1.70 meters tall, then the "error" is −0.05 meters. The expected value, being the mean of the entire population, is typically unobservable, and hence the statistical error cannot be observed either.

A **residual** (or fitting error), on the other hand, is an observable *estimate* of the unobservable statistical error. Consider the previous example with men's heights and suppose we have a random sample of *n* people. The *sample mean* could serve as a good estimator of the *population* mean. Then we have:

- The difference between the height of each man in the sample and the unobservable
*population*mean is a*statistical error*, whereas - The difference between the height of each man in the sample and the observable
*sample*mean is a*residual*.

Note that the sum of the residuals within a random sample is necessarily zero, and thus the residuals are necessarily *not independent*. The statistical errors on the other hand are independent, and their sum within the random sample is almost surely not zero.

One can standardize statistical errors (especially of a normal distribution) in a z-score (or "standard score"), and standardize residuals in a t-statistic, or more generally studentized residuals.

### Example

If we assume a normally distributed population with mean μ and standard deviation σ, and choose individuals independently, then we have

and the sample mean

is a random variable distributed thus:

The *statistical errors* are then

whereas the *residuals* are

(As is often done, the "hat" over the letter ε indicates an observable *estimate* of an unobservable quantity called ε.)

The sum of squares of the **statistical errors**, divided by σ^{2}, has a chi-squared distribution with *n* degrees of freedom:

This quantity, however, is not observable. The sum of squares of the **residuals**, on the other hand, is observable. The quotient of that sum by σ^{2} has a chi-squared distribution with only *n* − 1 degrees of freedom:

This difference between *n* and *n* − 1 degrees of freedom results in Bessel's correction for the estimation of sample variance of a population with unknown mean and unknown variance, though if the mean is known, no correction is necessary.

It is remarkable that the sum of squares of the residuals and the sample mean can be shown to be independent of each other, using, e.g. Basu's theorem. That fact, and the normal and chi-squared distributions given above, form the basis of calculations involving the quotient

The probability distributions of the numerator and the denominator separately depend on the value of the unobservable population standard deviation *σ*, but *σ* appears in both the numerator and the denominator and cancels. That is fortunate because it means that even though we do not know *σ*, we know the probability distribution of this quotient: it has a Student's t-distribution with *n* − 1 degrees of freedom. We can therefore use this quotient to find a confidence interval for *μ*.

## Regressions

In regression analysis, the distinction between *errors* and *residuals* is subtle and important, and leads to the concept of studentized residuals. Given an unobservable function that relates the independent variable to the dependent variable – say, a line – the deviations of the dependent variable observations from this function are the unobservable errors. If one runs a regression on some data, then the deviations of the dependent variable observations from the *fitted* function are the residuals.

However, a terminological difference arises in the expression mean squared error (MSE). The mean squared error of a regression is a number computed from the sum of squares of the computed *residuals*, and not of the unobservable *errors*. If that sum of squares is divided by *n*, the number of observations, the result is the mean of the squared residuals. Since this is a biased estimate of the variance of the unobserved errors, the bias is removed by multiplying the mean of the squared residuals by *n* / *df* where *df* is the number of degrees of freedom (*n* minus the number of parameters being estimated). This method gets exactly the same answer as the method using the mean of the squared error. This latter formula serves as an unbiased estimate of the variance of the unobserved errors, and is called the mean squared error.^{[1]}

Another method to calculate the means square of error when analyzing the variance of linear regression using a technique like that used in ANOVA (they are the same because ANOVA is a type of regression), the sum of squares of the residuals (aka sum of squares of the error) is divided by the degrees of freedom (where the degrees of freedom equals *n-p-1*, where p is the number of 'parameters' or predictors used in the model (i.e. the number of variables in the regression equation). One can then also calculate the mean square of the model by dividing the sum of squares of the model minus the degrees of freedom, which is just the number of parameters. Then the F value can be calculated by divided MS(model) by MS(error), and we can then determine significance (which is why you want the means squares to begin with.).^{[2]}

However, because of the behavior of the process of regression, the *distributions* of residuals at different data points (of the input variable) may vary *even if* the errors themselves are identically distributed. Concretely, in a linear regression where the errors are identically distributed, the variability of residuals of inputs in the middle of the domain will be *higher* than the variability of residuals at the ends of the domain: linear regressions fit endpoints better than the middle.
This is also reflected in the influence functions of various data points on the regression coefficients: endpoints have more influence.

Thus to compare residuals at different inputs, one needs to adjust the residuals by the expected variability of *residuals,* which is called studentizing. This is particularly important in the case of detecting outliers: a large residual may be expected in the middle of the domain, but considered an outlier at the end of the domain.

### Stochastic error

The stochastic error in a measurement is the error that is random from one measurement to the next. Stochastic errors tend to be gaussian (normal), in their distribution. That's because the stochastic error is most often the sum of many random errors, and when many random errors are added together, the distribution of their sum looks gaussian, as shown by the Central Limit Theorem. A stochastic error is added to a regression equation to introduce all the variation in Y that cannot be explained by the included Xs. It is, in effect, a symbol of our inability to model all the movements of the dependent variable.

## Other uses of the word "error" in statistics

The use of the term "error" as discussed in the sections above is in the sense of a deviation of a value from a hypothetical unobserved value. At least two other uses also occur in statistics, both referring to observable prediction errors:

Mean square error or **mean squared error** (abbreviated MSE) and root mean square error (RMSE) refer to the amount by which the values predicted by an estimator differ from the quantities being estimated (typically outside the sample from which the model was estimated).

**Sum of squared errors**, typically abbreviated SSE or SS_{e}, refers to the residual sum of squares (the sum of squared residuals) of a regression; this is the sum of the squares of the deviations of the actual values from the predicted values, within the sample used for estimation. Likewise, the **sum of absolute errors** (SAE) refers to the sum of the absolute values of the residuals, which is minimized in the least absolute deviations approach to regression.

## See also

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- Absolute deviation
- Consensus forecasts
- Deviation (statistics)
- Error detection and correction
- Explained sum of squares
- Innovation (signal processing)
- Innovations vector
- Lack-of-fit sum of squares
- Margin of error
- Mean absolute error
- Propagation of error
- Regression dilution
- Root mean square deviation
- Sampling error
- Studentized residual
- Type I and type II errors

## References

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