--- title: Some Applications subtitle: Biostat 216 author: Dr. Hua Zhou @ UCLA date: today format: html: theme: cosmo embed-resources: true number-sections: true toc: true toc-depth: 4 toc-location: left code-fold: false jupyter: jupytext: formats: 'ipynb,qmd' text_representation: extension: .qmd format_name: quarto format_version: '1.0' jupytext_version: 1.15.2 kernelspec: display_name: Julia 1.9.3 language: julia name: julia-1.9 --- ```{julia} using Pkg Pkg.activate(pwd()) Pkg.instantiate() Pkg.status() ``` ## Matrix completion Load the 128×128 Lena picture with missing pixels. ```{julia} using FileIO, Images lena = load("lena128missing.png") ``` ```{julia} # convert to real matrices Y = Float64.(lena) ``` We fill out the missing pixels uisng a **matrix completion** technique developed by Candes and Tao $$ \text{minimize } \|\mathbf{X}\|_* $$ $$ \text{subject to } x_{ij} = y_{ij} \text{ for all observed entries } (i, j). $$ Here $\|\mathbf{M}\|_* = \sum_i \sigma_i(\mathbf{M})$ is the nuclear norm. In words we seek the matrix with minimal nuclear norm that agrees with the observed entries. This is a semidefinite programming (SDP) problem readily solved by modern convex optimization software. We use the convex optimizaion package COSMO.jl to solve for this semi-definite program. ```{julia} # # Use COSMO solver using Convex, COSMO solver = COSMO.Optimizer() # Linear indices of obs. entries obsidx = findall(Y[:] .≠ 0.0) # Create optimization variables X = Variable(size(Y)) # Set up optmization problem problem = minimize(nuclearnorm(X)) problem.constraints += X[obsidx] == Y[obsidx] # Solve the problem by calling solve @time solve!(problem, solver) # fast ``` ```{julia} colorview(Gray, X.value) ``` ## Compressed sensing * **Compressed sensing** [Candes and Tao (2006)](https://doi.org/10.1109/TIT.2006.885507) and [Donoho (2006)](https://doi.org/10.1109/TIT.2006.871582) tries to address a fundamental question: how to compress and transmit a complex signal (e.g., musical clips, mega-pixel images), which can be decoded to recover the original signal? * Suppose a signal $\mathbf{x} \in \mathbb{R}^n$ is sparse with $s$ non-zeros. We under-sample the signal by multiplying a (flat) measurement matrix $\mathbf{y} = \mathbf{A} \mathbf{x}$, where $\mathbf{A} \in \mathbb{R}^{m\times n}$ has iid normal entries. [Candes, Romberg and Tao (2006)](https://doi.org/10.1002/cpa.20124) show that the solution to $$ \begin{eqnarray*} &\text{minimize}& \|\mathbf{x}\|_1 \\ &\text{subject to}& \mathbf{A} \mathbf{x} = \mathbf{y} \end{eqnarray*} $$ exactly recovers the true signal under certain conditions on $\mathbf{A}$ when $n \gg s$ and $m \approx s \ln(n/s)$. Why sparsity is a reasonable assumption? _Virtually all real-world images have low information content_. Generate a sparse signal and sub-sampling: ```{julia} using CairoMakie, Makie, Random # random seed Random.seed!(123) # Size of signal n = 1024 # Sparsity (# nonzeros) in the signal s = 10 # Number of samples (undersample by a factor of 8) m = 128 # Generate and display the signal x0 = zeros(n) x0[rand(1:n, s)] = randn(s) # Generate the random sampling matrix A = randn(m, n) / m # Subsample by multiplexing y = A * x0 # plot the true signal f = Figure() Makie.Axis( f[1, 1], title = "True Signal x0", xlabel = "x", ylabel = "y" ) lines!(1:n, x0) f ``` Solve the linear programming problem. ```{julia} # Use COSMO solver solver = COSMO.Optimizer() # MOI.set(solver, MOI.RawOptimizerAttribute("max_iter"), 5000) # Set up optimizaiton problem x = Variable(n) problem = minimize(norm(x, 1)) problem.constraints += A * x == y # Solve the problem @time solve!(problem, solver) ``` ```{julia} # Display the solution f = Figure() Makie.Axis( f[1, 1], title = "Reconstructed signal overlayed with x0", xlabel = "x", ylabel = "y" ) scatter!(1:n, x0, label = "truth") lines!(1:n, vec(x.value), label = "recovery") axislegend(position = :lt) f ``` ## Automatic differentiation (Auto-Diff) Last week we scratched the surface of matrix/vector calculus and chain rules. Recent surge of machine learning sparked rapid advancement of automatic differentiation, which applies chain rule to the computer code to obtain exact gradients (up to machine precision). ### Example: multivariate normal Define log-likelihood function. ```{julia} using Distributions, DistributionsAD, LinearAlgebra, PDMats, Random, Zygote Random.seed!(216) n, p = 100, 3 Y = randn(p, n) # each column of Y is a sample ``` ```{julia} # log-likelihood evaluator mnlogl = (θ) -> loglikelihood(MvNormal(θ[:μ], θ[:Ω]), Y) ``` ```{julia} # log-likelihood at (μ = 0, Ω = I) θ = (μ = zeros(p), Ω = Matrix{Float64}(I(p))) mnlogl(θ) ``` Calculate gradient by auto-diff. ```{julia} # gradient of log-likeliohod at (μ = 0, Ω = I) θ̄ = Zygote.gradient(mnlogl, θ)[1]; ``` ```{julia} θ̄[:μ] ``` ```{julia} θ̄[:Ω] ``` Let us check whether auto-diff yields the same answer as our analytical derivations. ```{julia} # analytical gradient dL/dμ = Ω^{-1} ∑ᵢ (yᵢ - μ) θ̄[:μ] ≈ θ[:Ω] \ sum(Y .- θ[:μ], dims = 2) ``` ```{julia} # analytical gradient dL/dΩ = -n/2 Ω^{-1} + 1/2 Ω^{-1} ∑ᵢ (yᵢ - μ)(yᵢ - μ)' Ω^{-1} θ̄[:Ω] ≈ - (n/2) * inv(θ[:Ω]) + 0.5 * inv(θ[:Ω]) * ((Y .- θ[:μ]) * (Y .- θ[:μ])') * inv(θ[:Ω]) ``` Surprise! Gradients of the covariance matrix do not match. Close inspection reveals that Julia calculates the gradient with respect to the upper triangular part of the covariance matrix $\text{vech}(\Omega)$ ```{julia} # gradient with respect to vech(Ω) θ̄[:Ω] ``` ```{julia} # gradient wrt vec(Ω) - (n/2) * inv(θ[:Ω]) + 0.5 * inv(θ[:Ω]) * ((Y .- θ[:μ]) * (Y .- θ[:μ])') * inv(θ[:Ω]) ``` ### Example: factor analysis Now let's try the more complicated factor analysis, where $\boldsymbol{\Omega} = \mathbf{F} \mathbf{F}' + \mathbf{D}$. ```{julia} # log-likelihood evaluator falogl = (θ) -> loglikelihood(MvNormal(θ[:F] * θ[:F]' + diagm(θ[:d])), Y) ``` ```{julia} r = 2 # log-likelihood at (F = ones(p, 2), d = ones(p)) θ = (F = ones(p, r), d = ones(p)) falogl(θ) ``` ```{julia} # gradient of log-likeliohod at (F = ones(p, 2), d = ones(p)) θ̄ = Zygote.gradient(falogl, θ)[1]; ``` ```{julia} # auto-diff gradient wrt F θ̄[:F] ``` ```{julia} # analytic gradient wrt F Ω = θ[:F] * θ[:F]' + diagm(θ[:d]) S = Y * Y' / n - n * inv(Ω) * θ[:F] + n * inv(Ω) * S * inv(Ω) * θ[:F] ``` ```{julia} # auto-diff gradient wrt d θ̄[:d] ``` ```{julia} # analytic gradient wrt d - (n / 2) * diag(inv(Ω) - inv(Ω) * S * inv(Ω)) ``` Hessian (second derivatives) is essentially gradient of gradient. ForwardDiff.jl is better for Hessian calculation. ```{julia} using ForwardDiff # HFF = ∂²L/∂F∂F' ForwardDiff.jacobian(F -> Zygote.gradient(falogl, (F = F, d = ones(p)))[1][:F], θ[:F]) ``` ```{julia} # Hdd = ∂²L/∂d∂d' ForwardDiff.jacobian(d -> Zygote.gradient(falogl, (F = θ[:F], d = d))[1][:d], θ[:d]) ``` ```{julia} # Hθθ = ∂²L/∂θ∂θ' # gradient function with vector input and vector output falogl_grad = function(θvec) θ = (F = reshape(θvec[1:(p * r)], p, r), d = θvec[(p * r + 1):(p * r + p)]) θ̄ = Zygote.gradient(falogl, θ)[1] return [vec(θ̄[:F]); vec(θ̄[:d])] end ForwardDiff.jacobian(falogl_grad, [vec(θ[:F]); vec(θ[:d])]) ```