Code


In 1886 Francis Galton published his observations about the height of children compared to their parents.

Defined mid-parent as the average of the heights of the parents.
When parents are taller or shorter than average, their children are more likely to be closer to the average height than their parents.
So called “regression to the mean.”
Galton fit a straight line to this effect, and the fitting of lines or curves to data has come to be called regression as well.
“I had so many colds last year, and then I started herbal remedies, and I have much fewer colds this year.”
“My investments were doing quite bad last year, so switched investment managers, and now it is doing much better.”
“The team had a terrible season, so we fired the coach – and this year they’re winning again.”
When in fact, they could be (at least partially) explained by:
Regression to the mean
The most common form of machine learning is regression, which means constructing an equation that describes the relationships among variables.
It is a form of supervised learning:
For example, we may look at these points and decide to model them using a line.
We may look at these points and decide to model them using a quadratic function.
ax = plt.figure(figsize = (5, 5)).add_subplot()
centerAxes(ax)
quad = np.array([1, 3, 0.5])
std = 8.0
np.random.seed(1)
xquad = -10.0 + 20.0 * np.random.random(100)
yquad = quad[0] + (quad[1] * xquad) + (quad[2] * xquad * xquad) + std * np.random.randn(100)
ax.plot(xquad, yquad, 'ro', markersize = 4)
plt.show()
And we may look at these points and decide to model them using a logarithmic function.
Clearly, none of these datasets agrees perfectly with the proposed model.
So the question arises:
How do we find the best linear function (or quadratic function, or logarithmic function) given the data?
This problem has been studied extensively in the field of statistics.
Certain terminology is used:
The basic regression task is:
The independent variables are collected into a matrix \(X,\) sometimes called the design matrix.
The dependent variables are collected into an observation vector \(\mathbf{y}.\)
The parameters of the model (for any kind of model) are collected into a parameter vector \(\boldsymbol\beta.\)
ax = plt.figure(figsize = (5, 5)).add_subplot()
centerAxes(ax)
line = np.array([1, 0.5])
np.random.seed(1)
xlin = -10.0 + 20.0 * np.random.random(100)
ylin = line[0] + (line[1] * xlin) + np.random.randn(100)
ax.plot(xlin, ylin, 'ro', markersize = 4)
ax.plot(xlin, line[0] + line[1] * xlin, 'b-')
plt.text(-9, 3, r'$y = \beta_0 + \beta_1x$', size=20)
plt.show()
The first kind of model we’ll study is a linear equation, \(y = \beta_0 + \beta_1 x.\)
Experimental data often produce points \((x_1, y_1), \dots, (x_n, y_n)\) that seem to lie close to a line.
We want to determine the parameters \(\beta_0, \beta_1\) that define a line that is as “close” to the points as possible.
Suppose we have a line \(y = \beta_0 + \beta_1 x\).
For each data point \((x_j, y_j),\) there is a point \((x_j, \beta_0 + \beta_1 x_j)\) that is the point on the line with the same \(x\)-coordinate.
def plot_residuals(x, y, beta_0, beta_1, figsize=(7, 4), title=None, legend=True):
# scatter the data, draw the line y = beta_0 + beta_1 x, and mark each residual
y_line = beta_0 + beta_1 * x
fig, ax = plt.subplots(figsize=figsize)
ax.scatter(x, y, color='blue', label='Data points', zorder=5)
ax.scatter(x, y_line, color='red', label='Predicted values', zorder=5)
ax.plot(x, y_line, color='cyan', label='Regression line (y = β0 + β1x)', zorder=4)
# residuals: vertical segments from each point to the line
for i in range(len(x)):
ax.vlines(x[i], y_line[i], y[i], color='blue', linestyles='dashed',
label='Residual' if i == 0 else "", zorder=2)
# label observed and predicted values, alternating above/below
y_offset = [0.2, -0.2, 0.2, -0.2, 0.2]
y_line_offset = [-0.3, 0.3, -0.3, 0.3, -0.2]
for i in range(len(x)):
ax.text(x[i], y[i] + y_offset[i], f'({x[i]}, {y[i]})', fontsize=9, ha='center')
ax.text(x[i], y_line[i] + y_line_offset[i], f'({x[i]}, {y_line[i]:.1f})', fontsize=9, ha='center')
ax.spines['top'].set_color('none')
ax.spines['right'].set_color('none')
ax.xaxis.set_ticks([])
ax.yaxis.set_ticks([])
if title:
ax.set_title(title)
if legend:
ax.legend()
return ax
x = np.array([1, 2, 3, 4, 5])
y = np.array([3.7, 2.0, 2.1, 0.1, 1.5])
plot_residuals(x, y, beta_0=4, beta_1=-0.8, title='Linear Regression with Residuals')
plt.show()

We call
The difference between an observed \(y\)-value and a predicted \(y\)-value is called a residual.
There are several ways to measure how “close” the line is to the data.
The usual choice is to sum the squares of the residuals.
The least-squares line is the line \(y = \beta_0 + \beta_1x\) that minimizes the sum of squares of the residuals.
The coefficients \(\beta_0, \beta_1\) of the line are called regression coefficients.
If the data points were on the line, the parameters \(\beta_0\) and \(\beta_1\) would satisfy the equations
\[ \begin{align*} \beta_0 + \beta_1 x_1 &= y_1, \\ \beta_0 + \beta_1 x_2 &= y_2, \\ \beta_0 + \beta_1 x_3 &= y_3, \\ &\vdots \\ \beta_0 + \beta_1 x_n &= y_n. \end{align*} \]
We can write this system as
\[ X\boldsymbol\beta = \mathbf{y}, \]
where
\[ X= \begin{bmatrix} 1 & x_1 \\ 1 & x_2 \\ \vdots & \vdots \\ 1 & x_n \end{bmatrix}, \;\;\boldsymbol\beta = \begin{bmatrix}\beta_0\\\beta_1\end{bmatrix}, \;\;\mathbf{y}=\begin{bmatrix}y_1\\y_2\\\vdots\\y_n\end{bmatrix}. \]
Of course, if the data points don’t actually lie exactly on a line,
… then there are no parameters \(\beta_0, \beta_1\) for which the predicted \(y\)-values in \(X\boldsymbol\beta\) equal the observed \(y\)-values in \(\mathbf{y}\),
… and \(X\boldsymbol\beta=\mathbf{y}\) has no solution.
Now, since the data doesn’t fall exactly on a line, we have decided to seek the \(\boldsymbol\beta\) that minimizes the sum of squared residuals, i.e.,
\[ \sum_i (\beta_0 + \beta_1 x_i - y_i)^2 =\Vert X\boldsymbol\beta -\mathbf{y}\Vert^2. \]
This is key:
Important
The sum of squares of the residuals is exactly the square of the distance between the vectors \(X\boldsymbol\beta\) and \(\mathbf{y}.\)
Computing the least-squares solution of \(X\boldsymbol\beta = \mathbf{y}\) is equivalent to finding the \(\boldsymbol\beta\) that determines the least-squares line.
ax = plt.figure(figsize = (5, 5)).add_subplot()
centerAxes(ax)
line = np.array([1, 0.5])
np.random.seed(1)
xlin = -10.0 + 20.0 * np.random.random(100)
ylin = line[0] + (line[1] * xlin) + np.random.randn(100)
ax.plot(xlin, ylin, 'ro', markersize = 4)
ax.plot(xlin, line[0] + line[1] * xlin, 'b-')
plt.text(-9, 3, r'$y = \beta_0 + \beta_1x$', size=20)
plt.show()
Now, to obtain the least-squares line, find the least-squares solution to \(X\boldsymbol\beta = \mathbf{y}.\)
Where does that solution come from? Not from a formula to memorize – from a picture.


The loss is the squared length of the residual, \(\lVert \mathbf{y} - X\boldsymbol\beta \rVert^2\). Its gradient is
\[ \nabla_{\boldsymbol\beta} \lVert \mathbf{y} - X\boldsymbol\beta \rVert^2 = -2\,X^T(\mathbf{y} - X\boldsymbol\beta), \]
and setting it to zero gives the previous slide’s condition:
\[ X^T(\mathbf{y} - X\hat{\boldsymbol\beta}) = \mathbf{0}. \]
The geometry says why it holds; the derivative gives an equation to solve. It is a minimum, not just a flat point, because the loss is a convex bowl.
Rearranging \(X^T(\mathbf{y} - X\hat{\boldsymbol\beta}) = \mathbf{0}\) gives the normal equations:
\[ X^TX\hat{\boldsymbol\beta} = X^T\mathbf{y}. \]
They say exactly this: the residual \(X\hat{\boldsymbol\beta} - \mathbf{y}\) is normal (i.e. orthogonal) to the column space of \(X\).
The normal equations always have at least one solution (\(X^T\mathbf{y}\) lies in the column space of \(X^T\), which equals the column space of \(X^TX\)).
If \(X^TX\) is invertible, the solution is unique:
\[ \hat{\boldsymbol\beta} = (X^TX)^{-1} X^T\mathbf{y}. \]
The five points from the residual plot, fit with \(y = \beta_0 + \beta_1 x\):
\[ X = \begin{bmatrix} 1 & 1 \\ 1 & 2 \\ 1 & 3 \\ 1 & 4 \\ 1 & 5 \end{bmatrix}, \qquad \mathbf{y} = \begin{bmatrix} 3.7 \\ 2.0 \\ 2.1 \\ 0.1 \\ 1.5 \end{bmatrix} \]
\[ X^TX = \begin{bmatrix} 5 & 15 \\ 15 & 55 \end{bmatrix}, \qquad X^T\mathbf{y} = \begin{bmatrix} 9.4 \\ 21.9 \end{bmatrix} \]
\[ \begin{aligned} 5\beta_0 + 15\beta_1 &= 9.4 \\ 15\beta_0 + 55\beta_1 &= 21.9 \end{aligned} \]
Triple the first and subtract:
\[ 10\beta_1 = -6.3 \;\Rightarrow\; \hat\beta_1 = -0.63, \quad \hat\beta_0 = 3.77 \]
Residual sum of squares: \(2.72\), below the \(3.4\) of the line we drew earlier.
Substitute \(\hat{\boldsymbol\beta}\) back into \(\hat{\mathbf{y}} = X\hat{\boldsymbol\beta}\):
\[ \hat{\mathbf{y}} = X(X^TX)^{-1}X^T\mathbf{y} = P\mathbf{y}. \]
\(P = X(X^TX)^{-1}X^T\) is the projection matrix, or hat matrix (it puts the hat on \(\mathbf{y}\)). It depends only on \(X\), not on \(\mathbf{y}\).
For \(X\) an \(n \times p\) matrix (\(n\) observations, \(p\) columns):
\[ X^TX \text{ is invertible} \iff X \text{ has full column rank, i.e. } \operatorname{rank}(X) = p, \]
meaning no column of \(X\) is a linear combination of the others.
This requires \(n \geq p\) (at least as many observations as columns), but \(n \ge p\) alone is not enough: two identical columns make \(X^TX\) singular at any \(n\).
When \(X^TX\) is singular the normal equations still have solutions – infinitely many. The fitted values \(\hat{\mathbf{y}} = P\mathbf{y}\) are still unique (the projection is), but the coefficients are not: the fit is determined, \(\boldsymbol\beta\) is not. Nearly collinear columns cause the same trouble in a milder form, which is where regularization comes in next lecture.
Another way that the inconsistent (i.e. no exact solution) linear system is often written is to collect all the residuals into a residual vector.
Then an exact equation is
\[ \mathbf{y} = X\boldsymbol\beta + \boldsymbol\epsilon, \]
where \(\boldsymbol\epsilon\) is the residual vector.
Any equation of this form is referred to as a linear model.
In this formulation, the goal is to find the \(\boldsymbol\beta\) so as to minimize the norm of \(\boldsymbol\epsilon\), i.e., \(\Vert\boldsymbol\epsilon\Vert.\)
In some cases, one would like to fit data points with something other than a straight line.
In cases like this, the matrix equation is still \(X\boldsymbol\beta = \mathbf{y}\), but the specific form of \(X\) changes from one problem to the next.
In model fitting, the parameters of the model are what is unknown.
A central question for us is whether the model is linear in its parameters.
For example, is this model linear in its parameters?
\[ y = \beta_0 e^{-\beta_1 x} \]
It is not linear in its parameters.
Is this model linear in its parameters?
\[ y = \beta_0 e^{-2 x} \]
It is linear in its parameters.
For a model that is linear in its parameters, an observation is a linear combination of (arbitrary) known functions.
In other words, a model that is linear in its parameters is
\[ y = \beta_0f_0(x) + \beta_1f_1(x) + \dots + \beta_{p-1}f_{p-1}(x) \]
where \(f_0, \dots, f_{p-1}\) are \(p\) known functions (they become the \(p\) columns of \(X\)) and \(\beta_0,\dots,\beta_{p-1}\) are parameters.
Suppose data points \((x_1, y_1), \dots, (x_n, y_n)\) appear to lie along some sort of parabola instead of a straight line.

As a result, we wish to approximate the data by an equation of the form
\[ y = \beta_0 + \beta_1x + \beta_2x^2. \]
Let’s describe the linear model that produces a “least squares fit” of the data by the equation.
The ideal relationship is \(y = \beta_0 + \beta_1x + \beta_2x^2.\)
Suppose the actual values of the parameters are \(\beta_0, \beta_1, \beta_2.\)
Then the coordinates of the first data point satisfy the equation
\[ y_1 = \beta_0 + \beta_1x_1 + \beta_2x_1^2 + \epsilon_1, \]
where \(\epsilon_1\) is the residual error between the observed value \(y_1\) and the predicted \(y\)-value.
Each data point determines a similar equation:
\[ \begin{align*} y_1 &= \beta_0 + \beta_1x_1 + \beta_2x_1^2 + \epsilon_1, \\ y_2 &= \beta_0 + \beta_1x_2 + \beta_2x_2^2 + \epsilon_2, \\ &\vdots \\ y_n &= \beta_0 + \beta_1x_n + \beta_2x_n^2 + \epsilon_n. \end{align*} \]
Clearly, this system can be written as \(\mathbf{y} = X\boldsymbol\beta + \boldsymbol\epsilon.\)
\[ \begin{bmatrix} y_1\\ y_2\\ \vdots\\ y_n \end{bmatrix} = \begin{bmatrix}1&x_1&x_1^2\\ 1&x_2&x_2^2\\ \vdots&\vdots&\vdots\\ 1&x_n&x_n^2 \end{bmatrix} \begin{bmatrix} \beta_0\\\ \beta_1\\\ \beta_2 \end{bmatrix} + \begin{bmatrix} \epsilon_1\\ \epsilon_2\\ \vdots\\ \epsilon_n \end{bmatrix} \]
Let’s solve for \(\boldsymbol\beta\), writing the formula out literally:
Don’t actually invert \(X^TX\)
np.linalg.inv(X.T @ X) @ X.T @ y mirrors the formula and is fine for a first look, but forming the inverse is numerically unstable when columns of \(X\) are nearly collinear – small rounding errors in \(X^TX\) become large errors in \(\hat{\boldsymbol\beta}\). From here on we use np.linalg.lstsq(X, y), which solves the same least-squares problem stably (via a QR or SVD factorization); np.linalg.solve(X.T @ X, X.T @ y) is the other common choice.
Now let’s try a different model.
\[ \begin{bmatrix} y_1\\ y_2\\ \vdots\\ y_n \end{bmatrix} = \begin{bmatrix}1&\log(x_1)\\ 1&\log(x_2)\\ \vdots&\vdots\\ 1&\log(x_n) \end{bmatrix} \begin{bmatrix} \beta_0\\\ \beta_1 \end{bmatrix} + \begin{bmatrix} \epsilon_1\\ \epsilon_2\\ \vdots\\ \epsilon_n \end{bmatrix} \]
Suppose an experiment involves two independent variables – say, \(u\) and \(v\), – and one dependent variable, \(y\).
A simple equation for predicting \(y\) from \(u\) and \(v\) has the form
\[ y = \beta_0 + \beta_1 u + \beta_2 v. \]
Since there is more than one independent variable, this is called multiple regression.
A more general prediction equation might have the form
\[ y = \beta_0 + \beta_1 u + \beta_2 v + \beta_3u^2 + \beta_4 uv + \beta_5 v^2. \]
A least squares fit to equations like this is called a trend surface.
In general, a linear model will arise whenever \(y\) is to be predicted by an equation of the form
\[ y = \beta_0f_0(u,v) + \beta_1f_1(u,v) + \cdots + \beta_{p-1}f_{p-1}(u,v), \]
with \(f_0,\dots,f_{p-1}\) any sort of known functions and \(\beta_0,\dots,\beta_{p-1}\) unknown weights.
Let’s take an example. Here are a set of points in \(\mathbb{R}^3\):
ax = ut.plotSetup3d(-7, 7, -7, 7, -10, 10, figsize = (5, 5))
v = [4.0, 4.0, 2.0]
u = [-4.0, 3.0, 1.0]
npts = 50
# set locations of points that fall within x,y
np.random.seed(1)
xc = -7.0 + 14.0 * np.random.random(npts)
yc = -7.0 + 14.0 * np.random.random(npts)
A = np.array([u,v]).T
# project these points onto the plane
P = A @ np.linalg.inv(A.T @ A) @ A.T
coords = P @ np.array([xc, yc, np.zeros(npts)])
coords[2] += np.random.randn(npts)
ax.plot(coords[0], coords[1], 'ro', zs=coords[2], markersize = 6)
plt.show()
In geography, local models of terrain are constructed from data
\[ (u_1, v_1, z_1), \dots, (u_n, v_n, z_n), \]
where \(u_j, v_j\), and \(z_j\) are latitude, longitude, and altitude, respectively.
Let’s describe the linear models that gives a least-squares fit to such data.
The solution is called the least-squares plane.
The model is \(z = \beta_0 + \beta_1 u + \beta_2 v + \epsilon\): altitude as a linear function of latitude and longitude. We expect the data to satisfy these equations:
\[ \begin{align*} z_1 &= \beta_0 + \beta_1 u_1 + \beta_2 v_1 + \epsilon_1, \\ z_2 &= \beta_0 + \beta_1 u_2 + \beta_2 v_2 + \epsilon_2, \\ \vdots \\ z_n &= \beta_0 + \beta_1 u_n + \beta_2 v_n + \epsilon_n. \end{align*} \]
This system has the matrix form \(\mathbf{z} = X\boldsymbol\beta + \boldsymbol\epsilon,\) with an \(n \times 3\) design matrix \(X\):
\[ \mathbf{z} = \begin{bmatrix}z_1\\ z_2\\ \vdots\\ z_n \end{bmatrix},\;\; X = \begin{bmatrix}1&u_1&v_1\\ 1&u_2&v_2\\ \vdots&\vdots&\vdots\\ 1&u_n&v_n \end{bmatrix},\;\; \boldsymbol\beta= \begin{bmatrix} \beta_0\\ \beta_1\\ \beta_2 \end{bmatrix},\;\; \boldsymbol\epsilon = \begin{bmatrix} \epsilon_1\\ \epsilon_2\\ \vdots\\ \epsilon_n \end{bmatrix}. \]
u_obs, v_obs, z_obs = coords
# design matrix [1, u, v] and the least-squares plane
X_plane = np.column_stack([np.ones(npts), u_obs, v_obs])
beta_plane, *_ = np.linalg.lstsq(X_plane, z_obs, rcond=None)
z_hat = X_plane @ beta_plane
ax = ut.plotSetup3d(-7, 7, -7, 7, -10, 10, figsize = (7, 7))
ax.set_xlabel('$u$', size=15)
ax.set_ylabel('$v$', size=15)
ax.set_zlabel('$z$', size=15)
# the fitted plane ...
uu, vv = np.meshgrid(np.linspace(-7, 7, 10), np.linspace(-7, 7, 10))
ax.plot_surface(uu, vv, beta_plane[0] + beta_plane[1] * uu + beta_plane[2] * vv,
color='green', alpha=0.3)
# ... and the residual from each point to it
for ui, vi, zi, zh in zip(u_obs, v_obs, z_obs, z_hat):
ax.plot([ui, ui], [vi, vi], [zi, zh], 'b-', lw=1)
ax.plot(u_obs, v_obs, 'ro', zs=z_obs, markersize=6)
plt.show()
The green surface is the fitted plane \(\hat z = \hat\beta_0 + \hat\beta_1 u + \hat\beta_2 v\); the blue segments are the residuals it minimizes (in the sum of squares).
This example shows that the linear model for multiple regression has the same form as the model for the simple regression in the earlier examples.
We can see that the general principle is the same across all the different kinds of linear models.
Once \(X\) is defined properly, the normal equations for \(\boldsymbol\beta\) have the same matrix form, no matter how many variables are involved.
Thus, for any linear model where \(X^TX\) is invertible, the least squares estimate is
\[ \hat{\boldsymbol\beta} = (X^TX)^{-1}X^T\mathbf{y}. \]
Given any \(X\) and \(\mathbf{y}\), the above algorithm will produce an output \(\hat{\boldsymbol\beta}\).
But how do we know whether the data is in fact well described by the model?
The most common measure of fit is \(R^2\).
\(R^2\) measures the fraction of the variance of \(\mathbf{y}\) that can be explained by the model \(X\hat{\boldsymbol\beta}\).
The variance of \(\mathbf{y}\) is
\[ \text{Var}(\mathbf{y}) =\frac{1}{n} \sum_{i=1}^n \left(y_i-\overline{y}\right)^2, \]
where \(\overline{y}=\frac{1}{n}\sum_{i=1}^ny_i\).
For any given \(n\), we can equally work with just \[ \sum_{i=1}^n \left(y_i-\overline{y}\right)^2, \]
which is called the Total Sum of Squares (TSS).
Now to measure the quality of fit of a model, we break TSS down into two components.
For any given \(\mathbf{x}_i\), the prediction made by the model is \(\hat{y_i} = \mathbf{x}_i^T\boldsymbol\beta\).
We can break the total sum of squares into two parts by adding and subtracting the predicted value \(\hat{y_i}\) for each \(i\):
\[ \sum_{i=1}^n \left[(y_i-\hat{y_i}) + (\hat{y_i}-\overline{y})\right]^2, \]
So we define the Residual Sum of Squares (RSS) as:
\[ \text{RSS} = \sum_{i=1}^n \left(y_i-\hat{y_i}\right)^2, \]
and the Explained Sum of Squares (ESS) as:
\[ \text{ESS} = \sum_{i=1}^n \left(\hat{y_i}-\overline{y}\right)^2, \]
One can show1 that the total sum of squares is exactly equal to the sum of squares of the residuals plus the sum of squares of the explained part.
In other words:
\[ \text{TSS} = \text{RSS} + \text{ESS}. \]
Now, a good fit is one in which the model explains a large part of the variance of \(\mathbf{y}\).
So the measure of fit \(R^2\) is defined as:
\[ R^2 = \frac{\text{ESS}}{\text{TSS}} = 1-\frac{\text{RSS}}{\text{TSS}} = 1 - \frac{\sum_{i=1}^n \left(y_i-\hat{y_i}\right)^2}{\sum_{i=1}^n \left(y_i-\overline{y}\right)^2}. \]
As a result, \(0\leq R^2\leq 1\) – on the training data, for a model with an intercept. That is what makes \(\text{TSS} = \text{RSS} + \text{ESS}\) hold.
Computed on held-out data (e.g. validation or test) (as r2_score does for Ames below) RSS can exceed TSS, and \(R^2\) can be negative: the model predicts worse than the constant \(\overline{y}\).
This is more specifically called the centered \(R^2\); it assumes an intercept. We will meet the uncentered variant in a moment, when a software package quietly switches to it.
The closer the value of \(R^2\) is to \(1\) the better the fit of the regression:
\(R^2\) is called the coefficient of determination.
It tells us “how well does the model predict the data?”
\(R^2\) is related to, but not the same thing as, Pearson’s correlation coefficient \(r\).
First, we’ll look at a test case on synthetic data. We’ll use Scikit-Learn’s make_regression function.
And then use the statsmodels package to fit the model.
And print the summary of the results.
OLS Regression Results
==============================================================================
Dep. Variable: y R-squared: 0.969
Model: OLS Adj. R-squared: 0.961
Method: Least Squares F-statistic: 124.5
Date: Fri, 16 Oct 2026 Prob (F-statistic): 2.66e-51
Time: 15:17:14 Log-Likelihood: -467.24
No. Observations: 100 AIC: 976.5
Df Residuals: 79 BIC: 1031.
Df Model: 20
Covariance Type: nonrobust
==============================================================================
coef std err t P>|t| [0.025 0.975]
------------------------------------------------------------------------------
const -4.2494 3.268 -1.300 0.197 -10.754 2.255
x1 11.5637 3.542 3.265 0.002 4.514 18.613
x2 -3.3068 2.835 -1.166 0.247 -8.950 2.336
x3 -1.8897 3.475 -0.544 0.588 -8.806 5.026
x4 2.4164 3.088 0.783 0.436 -3.730 8.563
x5 -2.2111 3.445 -0.642 0.523 -9.068 4.645
x6 1.0613 3.152 0.337 0.737 -5.213 7.336
x7 -2.9127 3.582 -0.813 0.419 -10.043 4.217
x8 90.5856 3.216 28.166 0.000 84.184 96.987
x9 -0.2241 3.389 -0.066 0.947 -6.970 6.522
x10 15.4059 3.236 4.761 0.000 8.965 21.847
x11 0.6029 3.385 0.178 0.859 -6.134 7.340
x12 0.8159 3.576 0.228 0.820 -6.302 7.933
x13 -0.2691 3.236 -0.083 0.934 -6.710 6.172
x14 90.6559 3.563 25.447 0.000 83.565 97.747
x15 1.0258 3.743 0.274 0.785 -6.425 8.477
x16 4.4945 2.731 1.646 0.104 -0.942 9.931
x17 9.9746 3.505 2.846 0.006 2.999 16.950
x18 72.9177 3.428 21.269 0.000 66.094 79.742
x19 -1.8957 3.500 -0.542 0.590 -8.861 5.070
x20 -0.8621 3.289 -0.262 0.794 -7.408 5.684
==============================================================================
Omnibus: 5.973 Durbin-Watson: 2.059
Prob(Omnibus): 0.050 Jarque-Bera (JB): 5.386
Skew: 0.483 Prob(JB): 0.0677
Kurtosis: 3.600 Cond. No. 2.67
==============================================================================
Notes:
[1] Standard Errors assume that the covariance matrix of the errors is correctly specified.
The \(R^2\) value is very good. We can see that the linear model does a very good job of predicting the observations \(y_i\).
Uncentered \(R^2\)
sm.OLS does not add an intercept for you – hence sm.add_constant. Fit sm.OLS(y, X) on the raw X instead and the summary switches to the uncentered \(R^2\),
\[ R^2 (\text{uncentered}) = 1 - \frac{\sum_{i=1}^n \left(y_i-\hat{y_i}\right)^2}{\sum_{i=1}^n y_i^2}, \]
and says so in a footnote. Without a constant column the residuals need not sum to zero, \(\text{TSS} = \text{RSS} + \text{ESS}\) fails and the centered \(R^2\) can be negative, so statsmodels divides by \(\sum y_i^2\) instead of \(\sum (y_i - \overline{y})^2\). The uncentered number is almost always larger and is not comparable to the centered one. Try it.
coef: \(\hat\beta_j\), the change in \(y\) per unit of \(x_j\) with the other columns held fixed.std err: \(\text{SE}(\hat\beta_j) = \sqrt{\hat\sigma^2\,[(X^TX)^{-1}]_{jj}}\), the uncertainty in that estimate.t and P>|t|: \(\hat\beta_j / \text{SE}\), and the probability of a \(t\) at least this large if the true coefficient were zero.[0.025 0.975]: the 95% confidence interval \(\hat\beta_j \pm t_{0.025,\,n-p}\,\text{SE}(\hat\beta_j)\). If it contains zero, the data cannot tell \(\beta_j\) from zero.R-squared and Adj. R-squared: fraction of variance explained; the adjusted version charges for each extra column, so it can go down.F-statistic: tests “every non-intercept coefficient is zero”.AIC, BIC: fit-minus-complexity scores for comparing models; lower is better.The full glossary is in the web notes under Aside: Summary Statistics.
Back to the example.
Some of the independent variables may not contribute to the accuracy of the prediction.
Each coefficient comes with a 95% confidence interval – the [0.025 0.975] columns of the table. Plotting them side by side makes the table readable at a glance:
coef = results.params
CIs = results.conf_int()
names = ['const'] + [f'$x_{{{j}}}$' for j in range(1, X.shape[1] + 1)] # match statsmodels' x1..x20
fig, ax = plt.subplots(figsize=(10, 4))
ax.errorbar(np.arange(len(coef)), coef,
yerr=[coef - CIs[:, 0], CIs[:, 1] - coef],
fmt='o', capsize=3, label='estimate with 95% CI')
ax.axhline(0, color='r', lw=1)
ax.set_xticks(np.arange(len(coef)))
ax.set_xticklabels(names)
ax.set_ylabel('coefficient')
ax.legend()
plt.show()
If a coefficient’s interval contains zero, the data cannot distinguish it from zero, and we cannot assume that there is any relationship between that independent variable and the observations. Six intervals sit clearly away from zero – but make_regression was told n_informative=5. One of the six is a false positive: at the 95% level, roughly one useless column in twenty will look significant by chance, and we have fifteen useless columns.
In other words, if the confidence interval for the parameter includes zero, the associated independent variable may not have any predictive value.
Confidence Intervals: [[-10.75360184 2.25481398]
[ 4.51429102 18.61312008]
[ -8.94962593 2.33603191]
[ -8.80586069 5.02646873]
[ -3.73021224 8.5631061 ]
[ -9.06769657 4.64546658]
[ -5.21308961 7.33575968]
[-10.04254055 4.2172332 ]
[ 84.18415371 96.98710861]
[ -6.96971003 6.52150734]
[ 8.96511318 21.84671808]
[ -6.13415773 7.33998878]
[ -6.301506 7.93330272]
[ -6.70975969 6.17158048]
[ 83.56490018 97.74693301]
[ -6.4252666 8.47684584]
[ -0.94153416 9.93061264]
[ 2.9990259 16.95023827]
[ 66.09389039 79.74158433]
[ -8.8614541 5.07001186]
[ -7.40787744 5.68373159]]
Parameters: [-4.24939393 11.56370555 -3.30679701 -1.88969598 2.41644693 -2.211115
1.06133504 -2.91265367 90.58563116 -0.22410134 15.40591563 0.60291552
0.81589836 -0.26908961 90.65591659 1.02578962 4.49453924 9.97463209
72.91773736 -1.89572112 -0.86207292]
Find the independent variables that are not significant.
array([False, False, True, True, True, True, True, True, False,
True, False, True, True, True, False, True, True, False,
False, True, True])
Let’s look at the shape of significant variables.
A tempting next step is to drop the columns whose interval covers zero and refit:
OLS Regression Results
==============================================================================
Dep. Variable: y R-squared: 0.966
Model: OLS Adj. R-squared: 0.964
Method: Least Squares F-statistic: 445.8
Date: Fri, 16 Oct 2026 Prob (F-statistic): 3.21e-66
Time: 15:17:14 Log-Likelihood: -471.66
No. Observations: 100 AIC: 957.3
Df Residuals: 93 BIC: 975.5
Df Model: 6
Covariance Type: nonrobust
==============================================================================
coef std err t P>|t| [0.025 0.975]
------------------------------------------------------------------------------
const -5.1888 2.927 -1.773 0.080 -11.001 0.623
x1 11.1097 3.161 3.515 0.001 4.833 17.386
x2 91.0034 2.685 33.890 0.000 85.671 96.336
x3 14.4371 2.891 4.993 0.000 8.696 20.179
x4 91.2173 3.273 27.868 0.000 84.717 97.717
x5 9.5400 3.072 3.105 0.003 3.439 15.641
x6 71.4542 3.080 23.201 0.000 65.338 77.570
==============================================================================
Omnibus: 10.945 Durbin-Watson: 2.133
Prob(Omnibus): 0.004 Jarque-Bera (JB): 13.411
Skew: 0.582 Prob(JB): 0.00122
Kurtosis: 4.366 Cond. No. 1.67
==============================================================================
Notes:
[1] Standard Errors assume that the covariance matrix of the errors is correctly specified.
Here that is nearly harmless – make_regression built \(y\) from five informative columns, and we kept those five plus one impostor. In general, though, be careful: choosing the features and judging the fit on the same data is the Lecture 7 anti-pattern. The refit looks better than it is, because the selection step already used the noise in this sample (that is exactly how the impostor got in).
Let’s see how powerful multiple regression can be on a real-world example.
A typical application of linear models is predicting house prices.
Linear models have been used for this problem for decades, and when a municipality does a value assessment on your house, they typically use a linear model.
We can consider various measurable attributes of a house (its “features”) as the independent variables, and the most recent sale price of the house as the dependent variable.
For our case study, we will use the features:
So our design matrix will have 8 columns (including the constant for the intercept):
\[ X\beta = \mathbf{y}, \]
and it will have one row for each house in the data set, with \(y\) the sale price of the house.
We will use data from housing sales in Ames, Iowa from 2006 to 2009:

Tim Kiser (w:User:Malepheasant) CC BY-SA 2.5 via Wikimedia Commons
import os, urllib.request
def data_file(path):
"""Course data file: use a local copy (here, or in the repo root above a
notebook in jupyter_notebooks/), else fetch it from the Materials repo (Colab)."""
for prefix in ('', '../'):
if os.path.exists(prefix + path):
return prefix + path
os.makedirs(os.path.dirname(path) or '.', exist_ok=True)
urllib.request.urlretrieve(
'https://raw.githubusercontent.com/tools4ds/DS701-Materials-FA26/main/' + path, path)
return path
df = pd.read_csv(data_file('data/ames-housing-data/train.csv'))| LotArea | GrLivArea | Fireplaces | FullBath | HalfBath | GarageArea | TotalBsmtSF | SalePrice | |
|---|---|---|---|---|---|---|---|---|
| 0 | 8450 | 1710 | 0 | 2 | 1 | 548 | 856 | 208500 |
| 1 | 9600 | 1262 | 1 | 2 | 0 | 460 | 1262 | 181500 |
| 2 | 11250 | 1786 | 1 | 2 | 1 | 608 | 920 | 223500 |
| 3 | 9550 | 1717 | 1 | 1 | 0 | 642 | 756 | 140000 |
| 4 | 14260 | 2198 | 1 | 2 | 1 | 836 | 1145 | 250000 |
Some things to note here:
Do we have scaling concerns here?
No, because each feature will get its own \(\beta\), which will correct for the scaling differences between different units of measure.
Note
Note that removing the intercept will cause the \(R^2\) to go up, which is counter-intuitive. The reason is explained here – but amounts to the fact that the formula for \(R^2\) with/without an intercept is different.
Let’s split the data into training and test sets.
Fit the model to the training data.
OLS Regression Results
==============================================================================
Dep. Variable: y R-squared: 0.759
Model: OLS Adj. R-squared: 0.757
Method: Least Squares F-statistic: 325.5
Date: Fri, 16 Oct 2026 Prob (F-statistic): 1.74e-218
Time: 15:17:15 Log-Likelihood: -8746.5
No. Observations: 730 AIC: 1.751e+04
Df Residuals: 722 BIC: 1.755e+04
Df Model: 7
Covariance Type: nonrobust
===============================================================================
coef std err t P>|t| [0.025 0.975]
-------------------------------------------------------------------------------
const -4.285e+04 5350.784 -8.007 0.000 -5.34e+04 -3.23e+04
LotArea 0.2361 0.131 1.798 0.073 -0.022 0.494
GrLivArea 48.0865 4.459 10.783 0.000 39.332 56.841
Fireplaces 1.089e+04 2596.751 4.192 0.000 5787.515 1.6e+04
FullBath 1.49e+04 3528.456 4.224 0.000 7977.691 2.18e+04
HalfBath 1.56e+04 3421.558 4.559 0.000 8882.381 2.23e+04
GarageArea 98.9856 8.815 11.229 0.000 81.680 116.291
TotalBsmtSF 62.6392 4.318 14.508 0.000 54.163 71.116
==============================================================================
Omnibus: 144.283 Durbin-Watson: 1.937
Prob(Omnibus): 0.000 Jarque-Bera (JB): 917.665
Skew: 0.718 Prob(JB): 5.39e-200
Kurtosis: 8.302 Cond. No. 6.08e+04
==============================================================================
Notes:
[1] Standard Errors assume that the covariance matrix of the errors is correctly specified.
[2] The condition number is large, 6.08e+04. This might indicate that there are
strong multicollinearity or other numerical problems.
We see that we have:
Why is a half bath ($15,600) worth more than a full bath ($14,900)?
Is our model doing a good job?
The summary table offers many statistics, but two pictures tell us more: the predictions against the ground truth, and then the residuals against the fitted values.
For each house we compute its predicted sale value according to our model:
\[ \hat{\mathbf{y}} = X\hat{\boldsymbol\beta} \]
from sklearn.metrics import r2_score
fig, (ax1, ax2) = plt.subplots(1,2,sharey = 'row', figsize=(12, 5))
y_oos_predict = results.predict(X_test)
r2_test = r2_score(y_test, y_oos_predict)
ax1.scatter(y_test, y_oos_predict, s = 8)
ax1.set_xlabel('True Price')
ax1.set_ylabel('Predicted Price')
ax1.plot([0,500000], [0,500000], 'r-')
ax1.axis('equal')
ax1.set_ylim([0, 500000])
ax1.set_xlim([0, 500000])
ax1.set_title(f'Out of Sample Prediction, $R^2$ is {r2_test:0.3f}')
#
y_is_predict = results.predict(X_train)
ax2.scatter(y_train, y_is_predict, s = 8)
r2_train = r2_score(y_train, y_is_predict)
ax2.set_xlabel('True Price')
ax2.plot([0,500000],[0,500000],'r-')
ax2.axis('equal')
ax2.set_ylim([0,500000])
ax2.set_xlim([0,500000])
ax2.set_title(f'In Sample Prediction, $R^2$ is {r2_train:0.3f}')
plt.show()Ignoring fixed x limits to fulfill fixed data aspect with adjustable data limits.
Ignoring fixed x limits to fulfill fixed data aspect with adjustable data limits.

We see that the model does a reasonable job in the middle of the price range, where most of the houses are.
At both ends the predictions are pulled toward the mean: cheap houses are over-predicted and expensive ones under-predicted. That is not a bug in this particular fit. \(\hat{\mathbf{y}}\) is a projection of \(\mathbf{y}\), so it is the shorter vector and \(\text{Var}(\hat{\mathbf{y}}) \le \text{Var}(\mathbf{y})\): fitted values are always less spread out than the truth. This is Galton’s regression to the mean, now falling out of the algebra.
Note that the \(R^2\) on the (held out) test data is 0.610, against 0.759 in sample. We are not doing as well on test data as on training data (somewhat to be expected).
\(R^2\) compresses the fit into one number; the residuals \(\mathbf{e} = \mathbf{y} - \hat{\mathbf{y}}\) show where the model is wrong. Plot them against the fitted values, again for the held-out houses:
