****************************************************************************** From: shaks@cfa237.harvard.edu (Jonathan Schachter) Message-Id: <9502180206.AA21071@cfa237.harvard.edu> To: scientists@cfa237.harvard.edu, postdocs@cfa237.harvard.edu, students@cfa237.harvard.edu, visitors@cfa237.harvard.edu Cc: msgs@cfa237.harvard.edu Subject: MIRIAD (radio astron.) software package now available on HEAD Date: Fri, 17 Feb 95 21:06:08 EST hi. with the aid of syshelp, i've made the MIRIAD radio astronomy software package (sun4 version) available in /soft/miriad. see below for how to start it up. DETAILS (skip now if you think this is junk email!): Most typically, MIRIAD is used for data from the VLA, the Australia Telescope Compact Array, the Hat Creek mm interferometer (BIMMA), and Westerbork (WSRT). Although AIPS can be used for VLA data, Compact Array and other data (linear feeds vs. circular for the VLA) where Stokes parameters are desired must be taken into MIRIAD for calibration and imaging. Usually, the data are flagged in AIPS, and then imported into MIRIAD. Unlike AIPS, MIRIAD has some important user friendly features: o direct, seamless access to a unix shell o data formats --- real disk files which can be archived with UNIX "tar" (instead of relatively bizarre-ly named VMS files in AIPS) o data analysis via shell scripts, freely mixing shell commands and miriad commands o command line editing and history (much like the T-shell) HOW TO RUN: 1. add these two lines to your .cshrc file (and then source it): source /soft/miriad/bin/MIRRC set path = ($MIRBIN $path) 2. start up "pgdisp" (/soft/xan/xanadu/sun4/bin/pgdisp if not already in your path) and "xmtv". note that "xmtv" shares the same socket as AIPS TV, so kill as necessary. 3. start up "miriad". 4. access online documentation with "help," see the manuals in /soft/miriad/man (postscript), or find me. jon schachter ****************************************************************************** Date: Thu, 16 Feb 95 23:09:31 EST From: shaks@cfa237.harvard.edu (Jonathan Schachter) Message-Id: <9502170409.AA16023@cfa237.harvard.edu> To: syshelp@cfa237.harvard.edu Subject: miriad installation Cc: ccarilli@cfa.harvard.edu, cgrant@cfa.harvard.edu, dharris@cfa.harvard.edu, jbookbinder@cfa.harvard.edu, shaks@cfa237.harvard.edu, taldcroft@cfa.harvard.edu dear syshelp (and copies to interested personnel): hi. i've now installed (in pool space) the sun4 version of miriad, a useful radio astronomy package. specifically, it does radio polarization data from the Australia Telescope (my current application) quite nicely. unlike AIPS, it can be driven purely via shell scripts, its terminal interface understands unix shell commands, and includes a line editing capability and history mechanism (like the unix T-shell). like AIPS, however, the data files do take up lots of disk space. i propose that miriad be installed in /soft/miriad/sun4. i can be the HEAD contact person. if there is sufficient interest, i can see about installing the solaris version as well, but first things first. all the relevant files are in /pool1/shaks. The total size is about 80 Megs. if you could please just copy those over to /soft/miriad/sun4. then please change the value of MIR in the file /soft/miriad/sun4/bin/MIRRC as follows: setenv MIR /soft/miriad/sun4 then, to run it, a user just needs to add these lines to his or her .cshrc file: source /soft/miriad/sun4/bin/MIRRC set path = ($MIRBIN $path) and then just type the word "miriad". two useful auxilliary programs are pgdisp, the PGPLOT server, and xmtv (like the AIPS TV). miriad uses the version of pgdisp already resident in our xanadu package (/soft/xan/xanadu/sun4/bin/pgdisp, or just pgdisp for those of us who already have xanadu in our path). xmtv is found in $MIRBIN. jon p.s. if there is an aipsusers mailing list, this might be circulated to that as well.