lmn_suff: Calculate the sufficient statistics of an LMN model.

View source: R/lmn_suff.R

lmn_suffR Documentation

Calculate the sufficient statistics of an LMN model.

Description

Calculate the sufficient statistics of an LMN model.

Usage

lmn_suff(Y, X, V, Vtype, npred = 0)

Arguments

Y

An n x q matrix of responses.

X

An N x p matrix of covariates, where N = n + npred (see Details). May also be passed as:

  • A scalar, in which case the one-column covariate matrix is X = X * matrix(1, N, 1). -X = 0, in which case the mean of Y is known to be zero, i.e., no regression coefficients are estimated.

V, Vtype

The between-observation variance specification. Currently the following options are supported:

  • Vtype = "full": V is an N x N symmetric positive-definite matrix.

  • Vtype = "diag": V is a vector of length N such that V = diag(V).

  • Vtype = "scalar": V is a scalar such that V = V * diag(N).

  • Vtype = "acf": V is either a vector of length N or an object of class SuperGauss::Toeplitz, such that V = toeplitz(V).

For V specified as a matrix or scalar, Vtype is deduced automatically and need not be specified.

npred

A nonnegative integer. If positive, calculates sufficient statistics to make predictions for new responses. See Details.

Details

The multi-response normal linear regression model is defined as

Y ~ Matrix-Normal(X B, V, Σ),

where Y_(n x q) is the response matrix, X_(n x p) is the covariate matrix, B_(p x q) is the coefficient matrix, V_(n x n) and Σ_(q x q) are the between-row and between-column variance matrices, and the Matrix-Normal distribution is defined by the multivariate normal distribution vec(Y) ~ N( vec(X B), Σ %x% V ), where vec(Y) is a vector of length nq stacking the columns of of Y, and Σ %x% V is the Kronecker product.

The function lmn_suff() returns everything needed to efficiently calculate the likelihood function

L(B, Σ | Y, X, V) = p(Y | X, V, B, Σ).

When npred > 0, define the variables Y_star = rbind(Y, y), X_star = rbind(X, x), and V_star = rbind(cbind(V, w), cbind(t(w), v)). Then lmn_suff() calculates summary statistics required to estimate the conditional distribution

p(y | Y, X_star, V_star, B, Σ).

The inputs to lmn_suff() in this case are Y = Y, X = X_star, and V = V_star.

Value

An S3 object of type lmn_suff, consisting of a list with elements:

Bhat

The p x q matrix B_hat = (X'V^{-1}X)^{-1}X'V^{-1}Y.

T

The p x p matrix T = X'V^{-1}X.

S

The q x q matrix S = (Y-X B_hat)'V^{-1}(Y-X B_hat).

ldV

The scalar log-determinant of V.

n, p, q

The problem dimensions, namely n = nrow(Y), p = nrow(Beta) (or p = 0 if X = 0), and q = ncol(Y).

In addition, when npred > 0 and with x, w, and v defined in Details:

Ap

The npred x q matrix A_p = w'V^{-1}Y.

Xp

The npred x p matrix X_p = x - w'V^{-1}X.

Vp

The scalar V_p = v - w'V^{-1}w.

Examples

# Data
n <- 50
q <- 3
Y <- matrix(rnorm(n*q),n,q)

# No intercept, diagonal V input
X <- 0
V <- exp(-(1:n)/n)
lmn_suff(Y, X = X, V = V, Vtype = "diag")

# X = (scaled) Intercept, scalar V input (no need to specify Vtype)
X <- 2
V <- .5
lmn_suff(Y, X = X, V = V)

# X = dense matrix, Toeplitz variance matrix
p <- 2
X <- matrix(rnorm(n*p), n, p)
Tz <- SuperGauss::Toeplitz$new(acf = 0.5*exp(-seq(1:n)/n))
lmn_suff(Y, X = X, V = Tz, Vtype = "acf")


mlysy/LMN documentation built on March 25, 2022, 11:12 a.m.