Solve weighted least squares (WLS) problem for a single lambda value
Solves the weighted least squares (WLS) problem for a single lambda value. Internal function that users should not call directly.
elnet.fit( x, y, weights, lambda, alpha = 1, intercept = TRUE, thresh = 1e-07, maxit = 1e+05, penalty.factor = rep(1, nvars), exclude = c(), lower.limits = -Inf, upper.limits = Inf, warm = NULL, from.glmnet.fit = FALSE, save.fit = FALSE )
x |
Input matrix, of dimension |
y |
Quantitative response variable. |
weights |
Observation weights. |
lambda |
A single value for the |
alpha |
The elasticnet mixing parameter, with 0 ≤ α ≤ 1. The penalty is defined as (1-α)/2||β||_2^2+α||β||_1.
|
intercept |
Should intercept be fitted (default=TRUE) or set to zero (FALSE)? |
thresh |
Convergence threshold for coordinate descent. Each inner
coordinate-descent loop continues until the maximum change in the objective
after any coefficient update is less than thresh times the null deviance.
Default value is |
maxit |
Maximum number of passes over the data; default is |
penalty.factor |
Separate penalty factors can be applied to each
coefficient. This is a number that multiplies |
exclude |
Indices of variables to be excluded from the model. Default is none. Equivalent to an infinite penalty factor. |
lower.limits |
Vector of lower limits for each coefficient; default
|
upper.limits |
Vector of upper limits for each coefficient; default
|
warm |
Either a |
from.glmnet.fit |
Was |
save.fit |
Return the warm start object? Default is FALSE. |
WARNING: Users should not call elnet.fit
directly. Higher-level functions
in this package call elnet.fit
as a subroutine. If a warm start object
is provided, some of the other arguments in the function may be overriden.
elnet.fit
is essentially a wrapper around a FORTRAN subroutine which
minimizes
1/2 ∑ w_i (y_i - X_i^T β)^2 + ∑ λ γ_j [(1-α)/2 β^2+α|β|],
over β, where γ_j is the relative penalty factor on the
jth variable. If intercept = TRUE
, then the term in the first sum is
w_i (y_i - β_0 - X_i^T β)^2, and we are minimizing over both
β_0 and β.
None of the inputs are standardized except for penalty.factor
, which
is standardized so that they sum up to nvars
.
An object with class "glmnetfit" and "glmnet". The list returned has
the same keys as that of a glmnet
object, except that it might have an
additional warm_fit
key.
a0 |
Intercept value. |
beta |
A |
df |
The number of nonzero coefficients. |
dim |
Dimension of coefficient matrix. |
lambda |
Lambda value used. |
dev.ratio |
The fraction of (null) deviance explained. The deviance calculations incorporate weights if present in the model. The deviance is defined to be 2*(loglike_sat - loglike), where loglike_sat is the log-likelihood for the saturated model (a model with a free parameter per observation). Hence dev.ratio=1-dev/nulldev. |
nulldev |
Null deviance (per observation). This is defined to be 2*(loglike_sat -loglike(Null)). The null model refers to the intercept model. |
npasses |
Total passes over the data. |
jerr |
Error flag, for warnings and errors (largely for internal debugging). |
offset |
Always FALSE, since offsets do not appear in the WLS problem. Included for compability with glmnet output. |
call |
The call that produced this object. |
nobs |
Number of observations. |
warm_fit |
If |
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