`MCMCvis` 0.13.1 – HPD intervals, multimodel visualization, and more!
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MCMCvis
version 0.13.1 is now on CRAN, complete with new features for summarizing and visualizing MCMC output. See HERE and HERE for posts that cover general package features. Highlights since the last CRAN version include:

MCMCsummary
– Specify quantiles for equaltailed credible intervals and return highest posterior density (HPD) intervals. MCMCplot
– Visualize posteriors from two different models on a single caterpillar plot. Useful when comparing parameter estimates across models and for visualizing shrinkage.MCMCplot
– Produce guide lines for caterpillar plots to more easily match parameter names to caterpillars.MCMCplot
– Specify colors for caterpillar plots. All functions – Summarize and visualize model output from
stanreg
objects produced with therstanarm
package andbrms
objects produced with thebrms
package (in addition to output produced with therstan
,rjags
,R2jags
, andjagsUI
packages).
Below we demonstrate how one might use some of these features using simulated data and simple models fit in JAGS.
Simulate some data
Let’s simulate data for 12 different groups using a generating process that assumes the means of these groups arise from a normal distribution with a constant mean and variance. In other words, we treat group as a ‘random effect’. We will make the groups differ in size to highlight how a random intercepts model will borrow strength compared to a model where groups are not modeled hierarchically, i.e. groups are treated as fixed effects.
# adapted from Marc Kery's WinBUGS for Ecologists (2010) set.seed(1) n_groups < 12 n_obs < rpois(n_groups, 8) n < sum(n_obs) mu_group < 20 sigma_group < 5 sigma < 8 alpha < rnorm(n_groups, mu_group, sigma_group) epsilon < rnorm(n, 0, sigma) x < rep(1:n_groups, n_obs) X < as.matrix(model.matrix(~as.factor(x) 1)) y < as.numeric(X %*% as.matrix(alpha) + epsilon) boxplot(y~x)
Fit two models to these data
First, let’s fit a simple means model to these data in JAGS where the means are not modeled hierarchically. We will use diffuse priors and let JAGS pick the initial values for simplicity’s sake.
{ sink("model1.R") cat(" model { # priors for (i in 1:n_groups) { alpha[i] ~ dnorm(0, 0.001) } sigma ~ dunif(0, 100) tau < 1 / sigma^2 # likelihood for (i in 1:n) { y[i] ~ dnorm(alpha[x[i]], tau) } } ", fill = TRUE) sink() } data < list(y = y, x = x, n = n, n_groups = n_groups) params < c("alpha", "sigma") gvals < c(alpha, sigma) jm < rjags::jags.model("model1.R", data = data, n.chains = 3, n.adapt = 5000) jags_out1 < rjags::coda.samples(jm, variable.names = params, n.iter = 10000
Next we fit a random intercepts model.
{ sink("model2.R") cat(" model { # priors for (i in 1:n_groups) { alpha[i] ~ dnorm(mu_group, tau_group) } mu_group ~ dnorm(0, 0.001) sigma_group ~ dunif(0, 100) tau_group < 1 / sigma_group^2 sigma ~ dunif(0, 100) tau < 1 / sigma^2 # likelihood for (i in 1:n) { y[i] ~ dnorm(alpha[x[i]], tau) } } ", fill = TRUE) sink() } data < list(y = y, x = x, n = n, n_groups = n_groups) params < c("alpha", "mu_group", "sigma", "sigma_group") gvals < c(alpha, mu_group, sigma, sigma_group) jm < rjags::jags.model("model2.R", data = data, n.chains = 3, n.adapt = 5000) jags_out2 < rjags::coda.samples(jm, variable.names = params, n.iter = 10000)
MCMCsummary
– custom equaltailed and HPD intervals
Sample quantiles in MCMCsummary
can now be specified directly using the probs
argument (removing the need to define custom quantiles with the func
argument). The default behavior is to provide 2.5%, 50%, and 97.5% quantiles. These probabilities can be changed by supplying a numeric vector to the probs
argument. Here we ask for 90% equaltailed credible intervals.
MCMCsummary(jags_out1, params = 'alpha', probs = c(0.1, 0.5, 0.9), round = 2) ## mean sd 10% 50% 90% Rhat n.eff ## alpha[1] 23.82 3.02 19.97 23.82 27.68 1 30385 ## alpha[2] 23.80 2.81 20.25 23.81 27.37 1 30000 ## alpha[3] 21.83 2.63 18.49 21.83 25.18 1 29699 ## alpha[4] 20.04 2.16 17.30 20.04 22.79 1 30000 ## alpha[5] 29.47 3.02 25.58 29.50 33.30 1 29980 ## alpha[6] 23.01 2.14 20.28 23.00 25.75 1 30305 ## alpha[7] 16.20 2.06 13.60 16.20 18.84 1 30000 ## alpha[8] 10.13 2.49 6.95 10.13 13.33 1 28967 ## alpha[9] 26.95 2.48 23.79 26.96 30.12 1 30000 ## alpha[10] 16.85 3.71 12.05 16.86 21.59 1 30262 ## alpha[11] 26.10 3.03 22.24 26.11 29.96 1 30473 ## alpha[12] 23.63 3.32 19.40 23.63 27.85 1 29627
Highest posterior density (HPD) intervals can now be displayed instead of equaltailed intervals by using HPD = TRUE
. This uses the HPDinterval
function from the coda
package to compute intervals based on the probability specified in the hpd_prob
argument (this argument is different than probs
argument, which is reserved for quantiles). Below we request 90% highest posterior density intervals.
MCMCsummary(jags_out1, params = 'alpha', HPD = TRUE, hpd_prob = 0.9, round = 2) ## mean sd 90%_HPDL 90%_HPDU Rhat n.eff ## alpha[1] 23.82 3.02 18.86 28.75 1 30385 ## alpha[2] 23.80 2.81 19.20 28.45 1 30000 ## alpha[3] 21.83 2.63 17.58 26.17 1 29699 ## alpha[4] 20.04 2.16 16.53 23.63 1 30000 ## alpha[5] 29.47 3.02 24.45 34.37 1 29980 ## alpha[6] 23.01 2.14 19.66 26.63 1 30305 ## alpha[7] 16.20 2.06 12.79 19.54 1 30000 ## alpha[8] 10.13 2.49 6.12 14.31 1 28967 ## alpha[9] 26.95 2.48 22.96 31.10 1 30000 ## alpha[10] 16.85 3.71 10.79 22.98 1 30262 ## alpha[11] 26.10 3.03 21.29 31.23 1 30473 ## alpha[12] 23.63 3.32 18.01 28.94 1 29627
MCMCplot
– multimodel visualization
Posterior estimates from two different models can also now be visualized with MCMCplot
. Let’s visually compare the alpha parameter posterior samples from the fixed effect and random intercepts models to see how our choice of model affected the posterior estimates. Below we can see that the random intercepts model means (in red) are pulled towards the true (generating value) grand mean (the vertical dashed line) compared to the fixed intercepts model means (in black), as expected due to shrinkage.
MCMCplot(object = jags_out1, object2 = jags_out2, params = 'alpha', offset = 0.2, ref = mu_group)
Guide lines can also be produced (using the guide_lines
argument) to help guide to eye from the parameter name to the associated caterpillar, which can be useful when trying to visualize a large number of parameters on a single plot. Colors can also be specified for each parameter (or the entire set of parameters).
MCMCplot(object = jags_out1, params = 'alpha', offset = 0.2, guide_lines = TRUE, ref = NULL, col = topo.colors(12), sz_med = 2.5, sz_thick = 9, sz_thin = 4)
Check out the full package vignette HERE. The MCMCvis
source code can be found HERE. More information on authors: Christian CheCastaldo, Casey Youngflesh.
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