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The most straightforward way to implement cross-validation in R for
statistical modeling functions that are written in the canonical manner
is to use update()
to refit the model with each fold
removed. This is the approach taken in the default method for
cv()
, and it is appropriate if the cases are independently
sampled. Refitting the model in this manner for each fold is generally
feasible when the number of folds in modest, but can be prohibitively
costly for leave-one-out cross-validation when the number of cases is
large.
The "lm"
and "glm"
methods for
cv()
take advantage of computational efficiencies by
avoiding refitting the model with each fold removed. Consider, in
particular, the weighted linear model \(\mathbf{y}_{n \times 1} = \mathbf{X}_{n \times
p}\boldsymbol{\beta}_{p \times 1} + \boldsymbol{\varepsilon}_{n \times
1}\), where \(\boldsymbol{\varepsilon}
\sim \mathbf{N}_n \left(\mathbf{0}, \sigma^2 \mathbf{W}^{-1}_{n \times
n}\right)\). Here, \(\mathbf{y}\) is the response vector, \(\mathbf{X}\) the model matrix, and \(\boldsymbol{\varepsilon}\) the error
vector, each for \(n\) cases, and \(\boldsymbol{\beta}\) is the vector of \(p\) population regression coefficients. The
errors are assumed to be multivariately normally distributed with 0
means and covariance matrix \(\sigma^2
\mathbf{W}^{-1}\), where \(\mathbf{W} =
\mathrm{diag}(w_i)\) is a diagonal matrix of inverse-variance
weights. For the linear model with constant error variance, the weight
matrix is taken to be \(\mathbf{W} =
\mathbf{I}_n\), the order-\(n\)
identity matrix.
The weighted-least-squares (WLS) estimator of \(\boldsymbol{\beta}\) is (see, e.g., Fox, 2016, sec. 12.2.2) 1 \[ \mathbf{b}_{\mathrm{WLS}} = \left( \mathbf{X}^T \mathbf{W} \mathbf{X} \right)^{-1} \mathbf{X}^T \mathbf{W} \mathbf{y} \]
Fitted values are then \(\widehat{\mathbf{y}} = \mathbf{X}\mathbf{b}_{\mathrm{WLS}}\).
The LOO fitted value for the \(i\)th case can be efficiently computed by \(\widehat{y}_{-i} = y_i - e_i/(1 - h_i)\) where \(h_i = \mathbf{x}^T_i \left( \mathbf{X}^T \mathbf{W} \mathbf{X} \right)^{-1} \mathbf{x}_i\) (the so-called “hatvalue”). Here, \(\mathbf{x}^T_i\) is the \(i\)th row of \(\mathbf{X}\), and \(\mathbf{x}_i\) is the \(i\)th row written as a column vector. This approach can break down when one or more hatvalues are equal to 1, in which case the formula for \(\widehat{y}_{-i}\) requires division by 0.
To compute cross-validated fitted values when the folds contain more than one case, we make use of the Woodbury matrix identity (Hager, 1989), \[ \left(\mathbf{A}_{m \times m} + \mathbf{U}_{m \times k} \mathbf{C}_{k \times k} \mathbf{V}_{k \times m} \right)^{-1} = \mathbf{A}^{-1} - \mathbf{A}^{-1}\mathbf{U} \left(\mathbf{C}^{-1} + \mathbf{VA}^{-1}\mathbf{U} \right)^{-1} \mathbf{VA}^{-1} \] where \(\mathbf{A}\) is a nonsingular order-\(n\) matrix. We apply this result by letting \[\begin{align*} \mathbf{A} &= \mathbf{X}^T \mathbf{W} \mathbf{X} \\ \mathbf{U} &= \mathbf{X}_\mathbf{j}^T \\ \mathbf{V} &= - \mathbf{X}_\mathbf{j} \\ \mathbf{C} &= \mathbf{W}_\mathbf{j} \\ \end{align*}\] where the subscript \(\mathbf{j} = (i_{j1}, \ldots, i_{jm})^T\) represents the vector of indices for the cases in the \(j\)th fold, \(j = 1, \ldots, k\). The negative sign in \(\mathbf{V} = - \mathbf{X}_\mathbf{j}\) reflects the removal, rather than addition, of the cases in \(\mathbf{j}\).
Applying the Woodbury identity isn’t quite as fast as using the
hatvalues, but it is generally much faster than refitting the model. A
disadvantage of the Woodbury identity, however, is that it entails
explicit matrix inversion and thus may be numerically unstable. The
inverse of \(\mathbf{A} = \mathbf{X}^T
\mathbf{W} \mathbf{X}\) is available directly in the
"lm"
object, but the second term on the right-hand side of
the Woodbury identity requires a matrix inversion with each fold
deleted. (In contrast, the inverse of each \(\mathbf{C} = \mathbf{W}_\mathbf{j}\) is
straightforward because \(\mathbf{W}\)
is diagonal.)
The Woodbury identity also requires that the model matrix be of full rank. We impose that restriction in our code by removing redundant regressors from the model matrix for all of the cases, but that doesn’t preclude rank deficiency from surfacing when a fold is removed. Rank deficiency of \(\mathbf{X}\) doesn’t disqualify cross-validation because all we need are fitted values under the estimated model.
glm()
computes the maximum-likelihood estimates for a
generalized linear model by iterated weighted least squares (see, e.g., Fox & Weisberg, 2019, sec.
6.12). The last iteration is therefore just a WLS fit of the
“working response” on the model matrix using “working weights.” Both the
working weights and the working response at convergence are available
from the information in the object returned by glm()
.
We then treat re-estimation of the model with a case or cases deleted
as a WLS problem, using the hatvalues or the Woodbury matrix identity.
The resulting fitted values for the deleted fold aren’t exact—that is,
except for the Gaussian family, the result isn’t identical to what we
would obtain by literally refitting the model—but in our (limited)
experience, the approximation is very good, especially for LOO CV, which
is when we would be most tempted to use it. Nevertheless, because these
results are approximate, the default for the "glm"
cv()
method is to perform the exact computation, which
entails refitting the model with each fold omitted.
Let’s compare the efficiency of the various computational methods for
linear and generalized linear models. Consider, for example,
leave-one-out cross-validation for the quadratic regression of
mpg
on horsepower
in the Auto
data, from the introductory “Cross-validating regression models”
vignette, repeated here:
data("Auto", package="ISLR2")
m.auto <- lm(mpg ~ poly(horsepower, 2), data = Auto)
summary(m.auto)
#>
#> Call:
#> lm(formula = mpg ~ poly(horsepower, 2), data = Auto)
#>
#> Residuals:
#> Min 1Q Median 3Q Max
#> -14.714 -2.594 -0.086 2.287 15.896
#>
#> Coefficients:
#> Estimate Std. Error t value Pr(>|t|)
#> (Intercept) 23.446 0.221 106.1 <2e-16 ***
#> poly(horsepower, 2)1 -120.138 4.374 -27.5 <2e-16 ***
#> poly(horsepower, 2)2 44.090 4.374 10.1 <2e-16 ***
#> ---
#> Signif. codes: 0 '***' 0.001 '**' 0.01 '*' 0.05 '.' 0.1 ' ' 1
#>
#> Residual standard error: 4.37 on 389 degrees of freedom
#> Multiple R-squared: 0.688, Adjusted R-squared: 0.686
#> F-statistic: 428 on 2 and 389 DF, p-value: <2e-16
library("cv")
summary(cv(m.auto, k = "loo") ) # default method = "hatvalues"
#> n-Fold Cross Validation
#> method: hatvalues
#> criterion: mse
#> cross-validation criterion = 19.248
summary(cv(m.auto, k = "loo", method = "naive"))
#> n-Fold Cross Validation
#> method: naive
#> criterion: mse
#> cross-validation criterion = 19.248
#> bias-adjusted cross-validation criterion = 19.248
#> full-sample criterion = 18.985
summary(cv(m.auto, k = "loo", method = "Woodbury"))
#> n-Fold Cross Validation
#> method: Woodbury
#> criterion: mse
#> cross-validation criterion = 19.248
#> bias-adjusted cross-validation criterion = 19.248
#> full-sample criterion = 18.985
This is a small regression problem and all three computational
approaches are essentially instantaneous, but it is still of interest to
investigate their relative speed. In this comparison, we include the
cv.glm()
function from the boot package
(Canty & Ripley, 2022; Davison & Hinkley,
1997), which takes the naive approach, and for which we have to
fit the linear model as an equivalent Gaussian GLM. We use the
microbenchmark()
function from the package of the same name
for the timings (Mersmann, 2023):
m.auto.glm <- glm(mpg ~ poly(horsepower, 2), data = Auto)
boot::cv.glm(Auto, m.auto.glm)$delta
#> [1] 19.248 19.248
microbenchmark::microbenchmark(
hatvalues = cv(m.auto, k = "loo"),
Woodbury = cv(m.auto, k = "loo", method = "Woodbury"),
naive = cv(m.auto, k = "loo", method = "naive"),
cv.glm = boot::cv.glm(Auto, m.auto.glm),
times = 10
)
#> Unit: milliseconds
#> expr min lq mean median uq max neval
#> hatvalues 1.3345 1.5178 1.5347 1.5442 1.5801 1.6284 10
#> Woodbury 14.9877 15.0436 15.2659 15.2147 15.4062 15.7366 10
#> naive 315.0382 316.9830 320.9941 321.9218 323.7760 330.4423 10
#> cv.glm 550.5770 557.5320 579.8248 565.4353 581.3043 666.1158 10
On our computer, using the hatvalues is about an order of magnitude faster than employing Woodbury matrix updates, and more than two orders of magnitude faster than refitting the model.2
Similarly, let’s return to the logistic-regression model fit to Mroz’s data on women’s labor-force participation, also employed as an example in the introductory vignette:
data("Mroz", package="carData")
m.mroz <- glm(lfp ~ ., data = Mroz, family = binomial)
summary(m.mroz)
#>
#> Call:
#> glm(formula = lfp ~ ., family = binomial, data = Mroz)
#>
#> Coefficients:
#> Estimate Std. Error z value Pr(>|z|)
#> (Intercept) 3.18214 0.64438 4.94 7.9e-07 ***
#> k5 -1.46291 0.19700 -7.43 1.1e-13 ***
#> k618 -0.06457 0.06800 -0.95 0.34234
#> age -0.06287 0.01278 -4.92 8.7e-07 ***
#> wcyes 0.80727 0.22998 3.51 0.00045 ***
#> hcyes 0.11173 0.20604 0.54 0.58762
#> lwg 0.60469 0.15082 4.01 6.1e-05 ***
#> inc -0.03445 0.00821 -4.20 2.7e-05 ***
#> ---
#> Signif. codes: 0 '***' 0.001 '**' 0.01 '*' 0.05 '.' 0.1 ' ' 1
#>
#> (Dispersion parameter for binomial family taken to be 1)
#>
#> Null deviance: 1029.75 on 752 degrees of freedom
#> Residual deviance: 905.27 on 745 degrees of freedom
#> AIC: 921.3
#>
#> Number of Fisher Scoring iterations: 4
summary(cv(m.mroz, # default method = "exact"
k = "loo",
criterion = BayesRule))
#> n-Fold Cross Validation
#> method: exact
#> criterion: BayesRule
#> cross-validation criterion = 0.32005
#> bias-adjusted cross-validation criterion = 0.3183
#> 95% CI for bias-adjusted CV criterion = (0.28496, 0.35164)
#> full-sample criterion = 0.30677
summary(cv(m.mroz,
k = "loo",
criterion = BayesRule,
method = "Woodbury"))
#> n-Fold Cross Validation
#> method: Woodbury
#> criterion: BayesRule
#> cross-validation criterion = 0.32005
#> bias-adjusted cross-validation criterion = 0.3183
#> 95% CI for bias-adjusted CV criterion = (0.28496, 0.35164)
#> full-sample criterion = 0.30677
summary(cv(m.mroz,
k = "loo",
criterion = BayesRule,
method = "hatvalues"))
#> n-Fold Cross Validation
#> method: hatvalues
#> criterion: BayesRule
#> cross-validation criterion = 0.32005
As for linear models, we report some timings for the various
cv()
methods of computation in LOO CV as well as for the
cv.glm()
function from the boot package
(which, recall, refits the model with each case removed, and thus is
comparable to cv()
with method="exact"
):
microbenchmark::microbenchmark(
hatvalues = cv(
m.mroz,
k = "loo",
criterion = BayesRule,
method = "hatvalues"
),
Woodbury = cv(
m.mroz,
k = "loo",
criterion = BayesRule,
method = "Woodbury"
),
exact = cv(m.mroz, k = "loo", criterion = BayesRule),
cv.glm = boot::cv.glm(Mroz, m.mroz,
cost = BayesRule),
times = 10
)
#> Unit: milliseconds
#> expr min lq mean median uq max neval
#> hatvalues 1.4388 1.6126 2.0269 1.6524 1.7319 5.273 10
#> Woodbury 47.5865 48.6913 49.6252 49.5880 50.1344 52.654 10
#> exact 2066.3274 2090.2715 2136.2337 2119.0919 2178.5412 2262.585 10
#> cv.glm 2452.5692 2477.5964 2527.5282 2540.4879 2543.2671 2644.205 10
There is a substantial time penalty associated with exact computations.
Let \(\mathrm{CV}(\mathbf{y}, \widehat{\mathbf{y}})\) represent a cross-validation cost criterion, such as mean-squared error, computed for all of the \(n\) values of the response \(\mathbf{y}\) based on fitted values \(\widehat{\mathbf{y}}\) from the model fit to all of the data. We require that \(\mathrm{CV}(\mathbf{y}, \widehat{\mathbf{y}})\) is the mean of casewise components, that is, \(\mathrm{CV}(\mathbf{y}, \widehat{\mathbf{y}}) = \frac{1}{n}\sum_{i=1}^n\mathrm{cv}(y_i, \widehat{y}_i)\).3 For example, \(\mathrm{MSE}(\mathbf{y}, \widehat{\mathbf{y}}) = \frac{1}{n}\sum_{i=1}^n (y_i - \widehat{y}_i)^2\).
We divide the \(n\) cases into \(k\) folds of approximately \(n_j \approx n/k\) cases each, where \(n = \sum n_j\). As above, let \(\mathbf{j}\) denote the indices of the cases in the \(j\)th fold.
Now define \(\mathrm{CV}_j = \mathrm{CV}(\mathbf{y}, \widehat{\mathbf{y}}^{(j)})\). The superscript \((j)\) on \(\widehat{\mathbf{y}}^{(j)}\) represents fitted values computed for all of the cases from the model with fold \(j\) omitted. Let \(\widehat{\mathbf{y}}^{(-i)}\) represent the vector of fitted values for all \(n\) cases where the fitted value for the \(i\)th case is computed from the model fit with the fold including the \(i\)th case omitted (i.e., fold \(j\) for which \(i \in \mathbf{j}\)).
Then the cross-validation criterion is just \(\mathrm{CV} = \mathrm{CV}(\mathbf{y}, \widehat{\mathbf{y}}^{(-i)})\). Following Davison & Hinkley (1997, pp. 293–295), the bias-adjusted cross-validation criterion is \[ \mathrm{CV}_{\mathrm{adj}} = \mathrm{CV} + \mathrm{CV}(\mathbf{y}, \widehat{\mathbf{y}}) - \frac{1}{n} \sum_{j=1}^{k} n_j \mathrm{CV}_j \]
We compute the standard error of CV as \[ \mathrm{SE}(\mathrm{CV}) = \frac{1}{\sqrt n} \sqrt{ \frac{\sum_{i=1}^n \left[ \mathrm{cv}(y_i, \widehat{y}_i^{(-i)} ) - \mathrm{CV} \right]^2 }{n - 1} } \] that is, as the standard deviation of the casewise components of CV divided by the square-root of the number of cases.
We then use \(\mathrm{SE}(\mathrm{CV})\) to construct a \(100 \times (1 - \alpha)\)% confidence interval around the adjusted CV estimate of error: \[ \left[ \mathrm{CV}_{\mathrm{adj}} - z_{1 - \alpha/2}\mathrm{SE}(\mathrm{CV}), \mathrm{CV}_{\mathrm{adj}} + z_{1 - \alpha/2}\mathrm{SE}(\mathrm{CV}) \right] \] where \(z_{1 - \alpha/2}\) is the \(1 - \alpha/2\) quantile of the standard-normal distribution (e.g, \(z \approx 1.96\) for a 95% confidence interval, for which \(1 - \alpha/2 = .975\)).
Bates, Hastie, & Tibshirani (2023) show that the coverage of this confidence interval is poor for small samples, and they suggest a much more computationally intensive procedure, called nested cross-validation, to compute better estimates of error and confidence intervals with better coverage for small samples. We may implement Bates et al.’s approach in a later release of the cv package. At present we use the confidence interval above for sufficiently large \(n\), which, based on Bates et al.’s results, we take by default to be \(n \ge 400\).
Consider calculating AUC for folds in which a validation set contains \(n_v\) observations. To calculate AUC in the validation set, we need the vector of prediction criteria, \(\widehat{\mathbf{y}}_{v_{(n_v \times 1)}} = (\widehat{y}_1, ..., \widehat{y}_{n_v})^T\), and the vector of observed responses in the validation set, \(\mathbf{y}_{v_{(n_v \times 1)}} = (y_1, \ldots, y_{n_v})^T\) with \(y_i \in \{0,1\}, \; i = 1, \ldots, n_v\).
To construct the ROC curve, only the ordering of the values in \(\mathbf{\widehat{y}}_v\) is relevant. Thus, assuming that there are no ties, and reordering observations if necessary, we can set \(\mathbf{\widehat{y}}_v = (1, 2, \ldots, n_v)^T\).
If the AUC can be expressed as the casewise mean or sum of a function \(\mathrm{cv}(\widehat{y}_i,y_i)\), where \(\mathrm{cv}: \{1,2,...,n_v\}\times\{0,1\} \rightarrow [0,1]\), then \[\begin{equation} \label{eq:cw} \tag{1} \sum_{i=1}^{n_v} \mathrm{cv}(\widehat{y}_i,y_i) = \mathrm{AUC}(\mathbf{\widehat{y}}_v,\mathbf{y}_v) \end{equation}\] must hold for all \(2^{n_v}\) possible values of \(\mathbf{y}_v = (y_1,...,y_{n_v})^T\). If all \(y\mathrm{s}\) have the same value, either 1 or 0, then the definition of AUC is ambiguous. AUC could be considered undefined, or it could be set to 0 if all \(y\)s are 0 and to 1 if all \(y\)s are 1. If AUC is considered to be undefined in these cases, we have \(2^{n_v} - 2\) admissible values for \(\mathbf{y}_v\).
Thus, equation (\(\ref{eq:cw}\)) produces either \(2^{n_v}\) or \(2^{n_v}-2\) constraints. Although there are only \(2n_v\) possible values for the \(\mathrm{cv(\cdot)}\) function, equation (\(\ref{eq:cw}\)) could, nevertheless, have consistent solutions. We therefore need to determine whether there is a value of \(n_v\) for which (\(\ref{eq:cw}\)) has no consistent solution for all admissible values of \(\mathbf{y}_v\). In that eventuality, we will have shown that AUC cannot, in general, be expressed through a casewise sum.
If \(n_v=3\), we show below that (\(\ref{eq:cw}\)) has no consistent solution if we include all possibilities for \(\mathbf{y}_v\), but does if we exclude cases where all \(y\)s have the same value. If \(n_v=4\), we show that there are no consistent solutions in either case.
The following R function computes AUC from \(\mathbf{\widehat{y}}_v\) and \(\mathbf{y}_v\), accommodating the cases where \(\mathbf{y}_v\) is all 0s or all 1s:
AUC <- function(y, yhat = seq_along(y)) {
s <- sum(y)
if (s == 0)
return(0)
if (s == length(y))
return(1)
Metrics::auc(y, yhat)
}
We then define a function to generate all possible \(\mathbf{y}_v\)s of length \(n_v\) as rows of the matrix \(\mathbf{Y}_{(2^{n_v} \times n_v)}\):
Ymat <- function(n_v, exclude_identical = FALSE) {
stopifnot(n_v > 0 &&
round(n_v) == n_v) # n_v must be a positive integer
ret <- sapply(0:(2 ^ n_v - 1),
function(x)
as.integer(intToBits(x)))[1:n_v,]
ret <- if (is.matrix(ret))
t(ret)
else
matrix(ret)
colnames(ret) <- paste0("y", 1:ncol(ret))
if (exclude_identical)
ret[-c(1, nrow(ret)),]
else
ret
}
For \(n_v=3\),
Ymat(3)
#> y1 y2 y3
#> [1,] 0 0 0
#> [2,] 1 0 0
#> [3,] 0 1 0
#> [4,] 1 1 0
#> [5,] 0 0 1
#> [6,] 1 0 1
#> [7,] 0 1 1
#> [8,] 1 1 1
If we exclude \(\mathbf{y}_v\)s with identical values, then
Ymat(3, exclude_identical = TRUE)
#> y1 y2 y3
#> [1,] 1 0 0
#> [2,] 0 1 0
#> [3,] 1 1 0
#> [4,] 0 0 1
#> [5,] 1 0 1
#> [6,] 0 1 1
Here is \(\mathbf{Y}\) with corresponding values of AUC:
cbind(Ymat(3), AUC = apply(Ymat(3), 1, AUC))
#> y1 y2 y3 AUC
#> [1,] 0 0 0 0.0
#> [2,] 1 0 0 0.0
#> [3,] 0 1 0 0.5
#> [4,] 1 1 0 0.0
#> [5,] 0 0 1 1.0
#> [6,] 1 0 1 0.5
#> [7,] 0 1 1 1.0
#> [8,] 1 1 1 1.0
The values of \(\mathrm{cv}(\widehat{y}_i, y_i)\) that express AUC as a sum of casewise values are solutions of equation (\(\ref{eq:cw}\)), which can be written as solutions of the following system of \(2^{n_v}\) linear simultaneous equations in \(2n_v\) unknowns: \[\begin{equation} \label{eq:lin} \tag{2} (\mathbf{U} -\mathbf{Y}) \mathbf{c}_0 + \mathbf{Y} \mathbf{c}_1 = [\mathbf{U} -\mathbf{Y}, \mathbf{Y}] \begin{bmatrix} \mathbf{c}_0 \\ \mathbf{c}_1 \end{bmatrix} = \mathrm{AUC}(\mathbf{\widehat{Y}},\mathbf{Y}) \end{equation}\] where \(\mathbf{U}_{(2^{n_v} \times n_v)}\) is a matrix of 1s conformable with \(\mathbf{Y}\); \(\mathbf{c}_0 = [\mathrm{cv}(1,0), c(2,0), ..., \mathrm{cv}(n_v,0)]^T\); \(\mathbf{c}_1 = [\mathrm{cv}(1,1), c(2,1), ..., \mathrm{cv}(n_v,1)]^T\); \([\mathbf{U} -\mathbf{Y}, \mathbf{Y}]_{(2^{n_v} \times 2n_v)}\) and \(\begin{bmatrix}\begin{aligned} \mathbf{c}_0 \\ \mathbf{c}_1 \end{aligned} \end{bmatrix}_{(2n_v \times 1)}\) are partitioned matrices; and \(\mathbf{\widehat{Y}}_{(2^{n_v} \times n_v)}\) is a matrix each of whose rows consists of the integers 1 to \(n_v\).
We can test whether equation (\(\ref{eq:lin}\)) has a solution for any given \(n_v\) by trying to solve it as a least-squares problem, considering whether the residuals of the associated linear model are all 0, using the “design matrix” \([\mathbf{U} -\mathbf{Y}, \mathbf{Y}]\) to predict the “outcome” \(\mathrm{AUC}(\mathbf{\widehat{Y}},\mathbf{Y})_{(2^{n_v} \times 1)}\):
resids <- function(n_v,
exclude_identical = FALSE,
tol = sqrt(.Machine$double.eps)) {
Y <- Ymat(n_v, exclude_identical = exclude_identical)
AUC <- apply(Y, 1, AUC)
X <- cbind(1 - Y, Y)
opts <- options(warn = -1)
on.exit(options(opts))
fit <- lsfit(X, AUC, intercept = FALSE)
ret <- max(abs(residuals(fit)))
if (ret < tol) {
ret <- 0
solution <- coef(fit)
names(solution) <- paste0("c(", c(1:n_v, 1:n_v), ",",
rep(0:1, each = n_v), ")")
attr(ret, "solution") <- zapsmall(solution)
}
ret
}
The case \(n_v=3\), excluding identical \(y\)s, has a solution:
resids(3, exclude_identical = TRUE)
#> [1] 0
#> attr(,"solution")
#> c(1,0) c(2,0) c(3,0) c(1,1) c(2,1) c(3,1)
#> 1.0 0.0 -0.5 0.5 0.0 0.0
But, if identical \(y\)s are included, the equation is not consistent:
For \(n_v=4\), there are no solutions in either case:
resids(4, exclude_identical = TRUE)
#> [1] 0.083333
resids(4, exclude_identical = FALSE)
#> [1] 0.25
Consequently, the widely employed AUC measure of fit for binary regression cannot in general be used for a casewise cross-validation criterion.
This is a definitional formula, which assumes that the
model matrix \(\mathbf{X}\) is of full
column rank, and which can be subject to numerical instability when
\(\mathbf{X}\) is ill-conditioned.
lm()
uses the singular-value decomposition of the model
matrix to obtain computationally more stable results.↩︎
Out of impatience, we asked
microbenchmark()
to execute each command only 10 times
rather than the default 100. With the exception of the last columns, the
output is self-explanatory. The last column shows which methods have
average timings that are statistically distinguishable. Because of the
small number of repetitions (i.e., 10), the "hatvalues"
and
"Woodbury"
methods aren’t distinguishable, but the
difference between these methods persists when we perform more
repetitions—we invite the reader to redo this computation with the
default times=100
repetitions.↩︎
Arlot & Celisse (2010) term the casewise loss, \(\mathrm{cv}(y_i, \widehat{y}_i)\), the “contrast function.”↩︎
These binaries (installable software) and packages are in development.
They may not be fully stable and should be used with caution. We make no claims about them.