similar to: How to solve ergodic density/distribution using R

Hi all, I would like to compute ergodic mean using MCMC output from WinBUGS. I tried using CODA package, but it seems that it is not implemented yet. Could anyone help me to compute this? Attached to this email are my output and index files. Kind regards, Raquel -- Raquel Rangel de Meireles Guimar?es Doutoranda em Demografia raquel at cedeplar.ufmg.br

Hi All, I have a problem trying to forecast using the dlm package, can anyone offer any advise? I setup my problem as follows, (following the manual as much as possible) data for example to run code CostUSD <- c(27.24031,32.97051, 38.72474, 22.78394, 28.58938, 49.85973, 42.93949, 35.92468) library(dlm) buildFun <- function(x) { dlmModPoly(1, dV = exp(x[1]), dW = exp(x[2])) } fit <-

Dear all, In many papers regarding time series analysis of acquired data, the authors analyze 'marginal distribution' (i.e. marginal with respect to time) of their data by for example checking 'cdf heavy tail' hypothesis. For i.i.d data this is ok, but what if samples are correlated, nonstationary etc.? Are there limit theorems which for example allow us to claim that

I am using the package hdrcde to get the highest density region. I have the data from an unknown distribution. And I used the subroutine hdr from the package to get the highest density region. But I always got a error message. I do not know why. Who can help?Thanks! The codes look like this: j is the data set, > hdr(j) Error in bw.SJ(x) : no solution in the specified range of bandwidths

To whom it may concern. As I would like to analyse some array data I was keen on downloading the lumi package that depends obviously on hdrcde that is not available for r 2.12.1. I did not find instructions to solve or circumvent this problem. Installing hdrcde by hand did not work either. It was not detected by > (.packages(all.available=TRUE)) if installed in the R library. Thanks Hermann

Dear R-help listers, Under the helps from the ggplot2 list, I have set up method of drawing a graph with multiple density plots arranged one by one in one page. Now, I want to add 95% confidential interval as vertical lines to x axe in density plot. I have found the library(hdrcde) can do this work, but I do not know how to handle functions of this library when I used ggplot2 to draw the graph.

Dear R-help listers, I want to add 95% confidential interval as vertical lines to x axe in density plot. I have found the library(hdrcde) can do this work, but I do not know how to handle functions of this library when I used ggplot2 to draw the graph. Thank you in advance. The data and codes followed: # dummy data factor<-rep(c("Alice","Jone","Mike"),each=100)

Dear All,   could you please confirm (or disconfimr, and then please explain:-)) my understanding of the results generated by the following code:   hdr.den(rnorm(200,55,3))   result:           [,1]     [,2] 99% 47.07170 63.26864 95% 48.83670 61.55108 50% 53.04884 57.37916   the way I am interpreting the results is that in this normally distributed data set with the mean of 55 and SD of 3:   1. 99%

> Hi, based on the multitude of answers and options received, you can also > consider the magnificent old days CDE, now open sourced. CDE can actually be installed on Centos 7 through yum: https://copr.fedorainfracloud.org/coprs/dcantrel/cde/ Just install the repo file and "yum install cde" That gives you CDE version 2.3. I installed it on an VirtualBox image that I use for

One of my users found that the new ssh-add, from the portable OpenSSH CVS as of October 12, was hanging in his .profile while trying to start up CDE (Common Desktop Environment) on Solaris 2.6. The previous one, which was from OpenSSH 2.9p2, did not hang. It turns out that CDE, at least on Solaris 2.6, 7 and 8, runs the user's .profile with a special startup shell that allocates a pseudo-tty

I''m new to puppet so this might be a foolish question. I''m using Solaris 10, server is Sparc, my client is x86. I created a ''file chown'' manifest as a test ... /etc/puppet/manifests/classes/puppet.pp class puppet { file { "/etc/puppet.txt": owner => "root", group => "root",

If you want to use row names to take a row subset of a data.frame then there is a bug when - One row has a name which is a completion of another row name - The shorter name comes after the longer one - You want to retrieve the row with the shorter name An example: R> x <- matrix(1:4, 2, 2, dimnames=list(c("abc","ab"), c("cde","cd"))) R> x cde

Hi Everyone, I am trying to access the gui on an OpenSolaris 200906 domU. dom0 is Solaris SXCE. I am following the below guide: http://opensolaris.org/os/community/xen/docs/setupvnc/ #################### - Turn on xdmcp. # svccfg -s cde-login svc:/application/graphical-login/cde-login> svc:/application/graphical-login/cde-login> setprop dtlogin/args=""

Hello, I recently bought a new Macbook Pro and installed R via a disk image from an older computer - it seems to work fine. I then installed the package "siar", tried to load it via the library command and received the following messages (note the "mvtnorm" package did not appear to load correctly): trying URL

I'm trying to configure my Solaris 9 pam.conf for CDE login/password expiration using ADS security on W2003. If my AD account password is in good standing, my config works great in /etc/pam.conf. However - I'm having trouble getting it to recognize that my password in AD has expired to ask me to reset it on the CDE screen. With the config below - it just tells me "login

On Thu, Jan 8, 2015 at 10:35 AM, Warren Young <wyml at etr-usa.com> wrote: >> > Would the world really be a better place if CDE had never been replaced? Me, I?ll take GNOME 3 and all its warts over CDE any day of the week. CDE never would have *evolved* to be the equal of GNOME; it had to be destroyed to make room. But it doesn't matter how pretty Gnome3 is on some other box.

libswfdec/swfdec_as_context.c | 20 + libswfdec/swfdec_as_interpret.c | 9 libswfdec/swfdec_as_string.c | 15 - libswfdec/swfdec_as_strings.c | 2 libswfdec/swfdec_as_types.c | 2 test/trace/Makefile.am | 28 + test/trace/isnan-5.swf |binary

Hi all, I am wondering how do I pull data from a remote host without running a daemon. PUSH command I would like the below statement be turned into a PULL from remote host instead. /usr/bin/rsync -e ssh --archive --sparse --compress --update --verbose --stats --progress --exclude=cdersync.tar.gz --exclude=*.bz2 --exclude=*.jpg --exclude=*.mp3 --exclude=ZDE --exclude=*.rpm --exclude=*.sit

On Thu, January 8, 2015 10:52 am, Les Mikesell wrote: > On Thu, Jan 8, 2015 at 10:35 AM, Warren Young <wyml at etr-usa.com> wrote: >>> >> Would the world really be a better place if CDE had never been replaced? >> Me, I???ll take GNOME 3 and all its warts over CDE any day of the week. >> CDE never would have *evolved* to be the equal of GNOME; it had to be

On Tue, 24 Sep, 2019 at 14:48:57 -0600, Frank Cox wrote: > On Tue, 24 Sep 2019 21:27:07 +0100 > Liam O'Toole wrote: > > > If the availability of a particular desktop environment is a > > showstopper, then perhaps RHEL and CentOS are not the best choice for > > you. > > That may be, but in view of the fact that you can even get a version of CDE that works