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From: Bayesian Models for Astrophysical Data, Cambridge Univ. Press

(c) 2017,  Joseph M. Hilbe, Rafael S. de Souza and Emille E. O. Ishida  

 

you are kindly asked to include the complete citation if you used this material in a publication

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Code 4.10 Normal linear model in R using JAGS and including errors in variables

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require(R2jags)


# Data
set.seed(1056)                                              # set seed to replicate example
nobs = 1000                                                 # number of obs in model

sdobsx <- 1.25


truex <- rnorm(nobs, 0, 2.5)                          # normal variable
errx <- rnorm(nobs, 0, sdobsx)
obsx <- truex + errx

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beta1 <- -4
beta2 <- 7
sdy <- 1.25
sdobsy <- 2.5

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erry <- rnorm(nobs, 0, sdobsy)
truey <- rnorm(nobs,beta1 + beta2*truex, sdy)
obsy <- truey + erry

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K <- 2

model.data <- list(obsy = obsy,
                             obsx = obsx,
                             K = K,
                             errx = errx,
                             erry = erry,
                             N = nobs)

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NORM_err <-" model{
    # Diffuse normal priors for predictors
    for (i in 1:K) { beta[i] ~ dnorm(0, 1e-3) }

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    # Uniform prior for standard deviation
    tauy <- pow(sigma, -2)                                      # precision
    sigma ~ dunif(0, 100)                                        # diffuse prior for standard deviation

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    # Diffuse normal priors for true x
    for (i in 1:N){
        x[i] ~ dnorm(0,1e-3)
    }

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    # Likelihood
    for (i in 1:N){
        obsy[i] ~ dnorm(y[i],pow(erry[i],-2))
        y[i] ~ dnorm(mu[i],tauy)
        obsx[i] ~ dnorm(x[i],pow(errx[i],-2))
        mu[i] <- beta[1]+beta[2]*x[i]
    }
}"

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# Initial values
inits <- function () {
    list(beta = rnorm(K, 0, 0.01))
}

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# Parameter to display and save
params <- c("beta", "sigma")

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evfit <- jags(data = model.data,
                     inits = inits,
                     parameters = params,
                     model = textConnection(NORM_err),
                     n.chains = 3,
                     n.iter = 5000,
                     n.thin = 1,
                     n.burnin = 2500)

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print(evfit,intervals=c(0.025, 0.975), digits=3)

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Output on screen:

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Inference for Bugs model at "3", fit using jags,

    3 chains, each with 5000 iterations (first 2500 discarded)

    n.sims = 7500 iterations saved

 

                      mu.vect      sd.vect             2.5%            97.5%        Rhat       n.eff

beta[1]             -4.069        0.135            -4.331            -3.806      1.007         620

beta[2]               6.753       0.058             6.636              6.862      1.008         280

sigma                 1.547       0.177             1.191              1.901      1.009         240

deviance      5391.166     51.448       5292.204        5492.494       1.001      6200

 

For each parameter, n.eff is a crude measure of effective sample size,

and Rhat is the potential scale reduction factor (at convergence, Rhat=1).

 

DIC info (using the rule, pD = var(deviance)/2)

pD = 1323.4 and DIC = 6714.5

DIC is an estimate of expected predictive error (lower deviance is better).

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