; CALDIR ;--------------------------------------------------------------- ;! lists calibrator source models available as AIPS FITS files ;# Verb calibration VLA ;----------------------------------------------------------------------- ;; Copyright (C) 2004, 2013, 2017, 2020 ;; Associated Universities, Inc. Washington DC, USA. ;; ;; This program is free software; you can redistribute it and/or ;; modify it under the terms of the GNU General Public License as ;; published by the Free Software Foundation; either version 2 of ;; the License, or (at your option) any later version. ;; ;; This program is distributed in the hope that it will be useful, ;; but WITHOUT ANY WARRANTY; without even the implied warranty of ;; MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the ;; GNU General Public License for more details. ;; ;; You should have received a copy of the GNU General Public ;; License along with this program; if not, write to the Free ;; Software Foundation, Inc., 675 Massachusetts Ave, Cambridge, ;; MA 02139, USA. ;; ;; Correspondence concerning AIPS should be addressed as follows: ;; Internet email: aipsmail@nrao.edu. ;; Postal address: AIPS Project Office ;; National Radio Astronomy Observatory ;; 520 Edgemont Road ;; Charlottesville, VA 22903-2475 USA ;----------------------------------------------------------------------- CALDIR LLLLLLLLLLLLUUUUUUUUUUUU CCCCCCCCCCCCCCCCCCCCCCCCCCCCC CALDIR: Verb to list all calibration source models available DATAIN To select Perley models from the web '2014', '2019' ---------------------------------------------------------------- CALDIR Type: Verb Use: Displays a list of all calibration models that may be read in with task CALRD. The Perley models are found on ftp.aoc.nrao.edu in directories pub/staff/rperley/MODELMAPS and pub/staff/rperley/MODELMAPS2019. Adverbs: DATAIN....If DATAIN begins with 'PERLEY' and contains 2014 or 2019 or is simply '2014' or '2019', then the available models listed are those found on the web in Rick Perley's 2014 or 2019 model sets. Any other value looks in the standard $AIPSTARS area on the local computer. See also: CALRD For the JVLA we are going to produce models at more closely spaced frequencies. One band so far has this done Name BAND actual frequency ---- ---- ---------------- S 2.1 2.141 GHz 2.7 2.663 3.0 3.047 3.5 3.463 3.8 3.847 ----------------------------------------------------------------