nmode's Git Repositories - Rnaught/blob - R/seqB.R

   1 #' seqB method
   2 #'
   3 #' This function implements a sequential Bayesian estimation method of R0 due to Bettencourt and Riberio (PloS One, 2008).  See details for important implementation notes.
   4 #'
   5 #'The method sets a uniform prior distribution on R0 with support (possible values) set from zero to \code{kappa}.  Our approach discretizes the distribution of R0 on a fine grid.   The distribution of R0 is then updated sequentially, with one update for each new case count observation.  The final estimate of R0 is \code{Rhat}, the mean of the (last) posterior distribution.
   6 #' The prior distribution is the initial belief of the distribution of R0; which in this implementation is the uninformative uniform distribution with values between zero and kappa.  Users can change the value of kappa only (ie. the prior distribution cannot be changed from the uniform).  As more case counts are observed, the influence of the prior distribution should lessen on the final estimate \code{Rhat}.
   7 #'
   8 #' This method is based on an approximation of the SIR model, which is most valid at the beginning of an epidemic.  The method assumes that the mean of the serial distribution (sometimes called the serial interval) is known.  The final estimate can be quite sensitive to this value, so sensitivity testing is recommended. Users should be careful about units of time (e.g. are counts observed daily or weekly?) when implementing.
   9 #'
  10 #' Our code has been modified to provide an estimate even if case counts equal to zero are present in some time intervals.  This is done by grouping the counts over such periods of time.  Without grouping, and in the presence of zero counts, no estimate can be provided.
  11 #'
  12 #' @param NT Vector of case counts
  13 #' @param mu Mean of the serial distribution (needs to match case counts in time units; for example, if case counts are weekly and the serial distribution has a mean of seven days, then mu should be set to 1)
  14 #' @param kappa Largest possible value of uniform prior, defaults to 20.
  15 #'
  16 #' @return secB returns a list containing the following components:  \code{Rhat} is the estimate of R0 (the posterior mean), \code{posterior} is the posterior distribution of R0 from which alternate estimates can be obtained (see examples), \code{group} is an indicator variable (if \code{group=TRUE}, zero values of NT were input and grouping was done to obtain \code{Rhat}), and \code{inputs} is a list of the original input variables \code{NT, gamma, kappa}.  The variable \code{posterior} is returned as a list made up of \code{supp} the support of the distribution and \code{pmf} the probability mass function.
  17 #'
  18 #' @examples
  19 #'
  20 #' ## ===================================================== ##
  21 #' ## Illustrate on weekly data                             ##
  22 #' ## ===================================================== ##
  23 #'
  24 #' NT <- c(1, 4, 10, 5, 3, 4, 19, 3, 3, 14, 4)
  25 #' ## obtain Rhat when serial distribution has mean of five days
  26 #' res1 <- seqB(NT=NT, mu=5/7)
  27 #' res1$Rhat
  28 #' ## obtain Rhat when serial distribution has mean of three days
  29 #' res2 <- seqB(NT=NT, mu=3/7)
  30 #' res2$Rhat
  31 #'
  32 #' ## ===================================================== ##
  33 #' ## Compute posterior mode instead of posterior mean      ##
  34 #' ## ===================================================== ##
  35 #'
  36 #' Rpost <-     res1$posterior
  37 #' loc <- which(Rpost$pmf==max(Rpost$pmf))
  38 #' Rpost$supp[loc]              # posterior mode
  39 #' res1$Rhat            # compare with posterior mean
  40 #'
  41 #' par(mfrow=c(2,1), mar=c(2,2,1,1))
  42 #' plot(Rpost$supp, Rpost$pmf, col="black", type="l", xlab="", ylab="")
  43 #' abline(h=1/(20/0.01+1), col="red")
  44 #' abline(v=res1$Rhat, col="blue")
  45 #' abline(v=Rpost$supp[loc], col="purple")
  46 #' legend("topright", legend=c("prior", "posterior", "posterior mean (Rhat)", "posterior mode"), col=c("red", "black", "blue", "purple"), lty=1)
  47 #' plot(Rpost$supp, Rpost$pmf, col="black", type="l", xlim=c(0.5,1.5), xlab="", ylab="")
  48 #' abline(h=1/(20/0.01+1), col="red")
  49 #' abline(v=res1$Rhat, col="blue")
  50 #' abline(v=Rpost$supp[loc], col="purple")
  51 #' legend("topright", legend=c("prior", "posterior", "posterior mean (Rhat)", "posterior mode"), col=c("red", "black", "blue", "purple"), lty=1)
  52 #'
  53 #' ## ========================================================= ##
  54 #' ## Compute Rhat using only the first five weeks of data      ##
  55 #' ## ========================================================= ##
  56 #'
  57 #'
  58 #' res3 <- seqB(NT=NT[1:5], mu=5/7)     # serial distribution has mean of five days
  59 #' res3$Rhat
  60 #' @export
  61
  62 seqB            <-      function(NT, mu, kappa=20){
  63
  64         gamma   <-      1/mu
  65
  66         if(length(NT)<2) {
  67                 print("Warning: length of NT should be at least two.")
  68         }
  69         else{
  70         if(min(NT)>0){
  71                 times           <-      1:length(NT)
  72                 tau                     <-      diff(times)
  73         }
  74
  75         group                   <-      FALSE
  76
  77         if(min(NT)==0){
  78                 times   <-      which(NT>0)
  79                 NT              <-      NT[times]
  80                 tau             <-      diff(times)
  81                 group   <-      TRUE
  82         }
  83
  84         R                       <-      seq(0, kappa, 0.01)
  85         prior0          <-      rep(1,kappa/0.01+1)
  86         prior0          <-      prior0/sum(prior0)
  87
  88         k                       <-      length(NT)-1
  89         R0.post         <-      matrix(0, nrow=k, ncol=length(R))
  90
  91         prior           <-      prior0
  92         posterior       <-      seq(0, length(prior0))
  93
  94         for(i in 1:k){
  95
  96         mm1                     <-      NT[i]
  97         mm2                     <-      NT[i+1]
  98         lambda          <-      tau[i]*gamma*(R-1)
  99         lambda          <-      log(mm1)+lambda
 100         loglik          <-      mm2*lambda-exp(lambda)
 101
 102 # numerical issues solve???
 103
 104 #       if((mm1==0)*(mm2==0)==0){
 105         maxll                   <-      max(loglik)
 106         const                   <-      0
 107         if(maxll>700){
 108         const                   <-      maxll-700
 109                 }
 110         loglik                  <-      loglik-const
 111 #       }
 112
 113 # end numerical issues solve???
 114
 115         posterior       <-      exp(loglik)*prior
 116         posterior       <-      posterior/sum(posterior)
 117
 118
 119         prior           <-      posterior
 120
 121         }
 122
 123         Rhat            <-      sum(R*posterior)
 124
 125 return(list(Rhat=Rhat, posterior=list(supp=R, pmf=posterior), group=group, inputs=list(NT=NT, mu=mu, kappa=kappa)))
 126 }
 127 }
 128
 129