In statistics, simple linear regression is the least squares estimator of a linear regression model with a single explanatory variable. In other words, simple linear regression fits a straight line through the set of n points in such a way that makes the sum of squared residuals of the model (that is, vertical distances between the points of the data set and the fitted line) as small as possible.
The adjective simple refers to the fact that this regression is one of the simplest in statistics. The fitted line has the slope equal to the correlation between y and x corrected by the ratio of standard deviations of these variables. The intercept of the fitted line is such that it passes through the center of mass (x, y) of the data points.
Other regression methods besides the simple ordinary least squares (OLS) also exist (see linear regression model). In particular, when one wants to do regression by eye, people usually tend to draw a slightly steeper line, closer to the one produced by the total least squares method. This occurs because it is more natural for one's mind to consider the orthogonal distances from the observations to the regression line, rather than the vertical ones as OLS method does.
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Suppose there are n data points {yi, xi}, where i = 1, 2, …, n. The goal is to find the equation of the straight line
which would provide a "best" fit for the data points. Here the "best" will be understood as in the least-squares approach: such a line that minimizes the sum of squared residuals of the linear regression model. In other words, numbers α and β solve the following minimization problem:
By using either calculus, the geometry of inner product spaces or simply expanding to get a quadratic in α and β, it can be shown that the values of α and β that minimize the objective function Q are
where rxy is the sample correlation coefficient between x and y, sx is the standard deviation of x, and sy is correspondingly the standard deviation of y. Horizontal bar over a variable means the sample average of that variable. For example:
Substituting the above expressions for and into
yields
This shows the role plays in the regression line of standardized data points.
Sometimes, people consider a simple linear regression model without the intercept term: y = βx. In such a case, the OLS estimator for β simplifies to .
If the have independent, non-uniform variances , then the function Q above becomes
However, the OLS estimators for α and β are still given by the same equations as above,
except with the averages computed as weighted means of the appropriate variable combinations.
The above equations assume that {xi} data are known exactly whereas {yi} data have random distribution. In case that both {xi} and {yi} are random we can minimize the orthogonal distances from the observations to the regression line (total least squares method). Here we will show equation for simple linear regression model without the intercept term y = βx under the assumption that x and y have equal variances. For general case please see Deming regression.
The orthogonal distance from the observation point {yi, xi} to the regression line y = βx is:
where denotes absolute value.
We will minimize sum of squared distances:
This can be solved by searching for which derivation is zero.
This yields the equation
Which has the solution:
Please note that there are two different solutions (note in the equation above). One solution represent minimum of function and the other one maximum of function. The corresponding lines are orthogonal to each other. For and for all i use + sign to get the slope of the regression line.
It can be shown that if you swap and you will get slope . This is not the case for simple linear regression without the intercept term which is using ordinary least squares method.
The formulas given in the previous section allow one to calculate the point estimates of α and β — that is, the coefficients of the regression line for the given set of data. However, those formulas do not tell us how precise the estimates are. That is, how much the estimators and can deviate from the "true" values of α and β. The latter question is answered by the confidence intervals for the regression coefficients.
In order to construct the confidence intervals usually one of the two possible assumptions is made: either that the errors in the regression are normally distributed (the so-called classic regression assumption), or that the number of observations n is sufficiently large so that the actual distribution of the estimators can be approximated using the Central Limit Theorem.
Under the first assumption above, that of the normality of the error terms, the estimator of the slope coefficient will itself be normally distributed with mean β and variance where is the variance of the error terms. At the same time the sum of squared residuals Q is distributed proportionally to χ2 with (n−2) degrees of freedom, and independently from This allows us to construct a t-statistic
which has a Student's t-distribution with (n−2) degrees of freedom. Here sβ is the standard deviation of the estimator
Using this t-statistic we can construct a confidence interval for β:
where is the (1−γ/2)-th quantile of the tn–2 distribution. For example, if γ = 0.05 then the confidence level is 95%.
Similarly, the confidence interval for the intercept coefficient α is given by
where
The confidence intervals for α and β give us the general idea where these regression coefficients are most likely to be. For example in the "Okun's law" regression shown at the beginning of the article the point estimates are and The 95% confidence intervals for these estimates are
In order to represent this information graphically, in the form of the confidence bands around the regression line, one has to proceed carefully and account for the joint distribution of the estimators. It can be shown that at confidence level (1−γ) the confidence band has hyperbolic form given by the equation
The alternative second assumption states that when the number of points in the dataset is "large enough", the Law of large numbers and the Central limit theorem become applicable, and then the distribution of the estimators is approximately normal. Under this assumption all formulas derived in the previous section remain valid, with the only exception that the quantile t*n−2 of student-t distribution is replaced with the quantile q* of the standard normal distribution. Occasionally the fraction 1⁄(n−2) is replaced with 1⁄n. When n is large such change does not alter the results considerably.
As an example we shall consider the data set from the Ordinary least squares article. This data set gives average weights for humans as a function of their height in the population of American women of age 30–39. Although the OLS article argues that it would be more appropriate to run a quadratic regression for this data, we will not do so and fit the simple linear regression instead.
xi | 1.47 | 1.50 | 1.52 | 1.55 | 1.57 | 1.60 | 1.63 | 1.65 | 1.68 | 1.70 | 1.73 | 1.75 | 1.78 | 1.80 | 1.83 | Height (m) |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
yi | 52.21 | 53.12 | 54.48 | 55.84 | 57.20 | 58.57 | 59.93 | 61.29 | 63.11 | 64.47 | 66.28 | 68.10 | 69.92 | 72.19 | 74.46 | Mass (kg) |
There are n = 15 points in this data set, and we start by calculating the following five sums:
These quantities can be used to calculate the estimates of the regression coefficients, and their standard errors.
The 0.975 quantile of Student's t-distribution with 13 degrees of freedom is t*13 = 2.1604, and thus confidence intervals for α and β are
This example also demonstrates that sophisticated calculations will not overcome the use of badly prepared data. The heights were originally given in inches, and have been converted to the nearest centimetre. Since the conversion factor is one inch to 2.54cm, this is not a correct conversion. The original inches can be recovered by Round(x/0.0254) and then re-converted to metric: if this is done, the results become
Thus a seemingly small variation in the data has a real effect.
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