; QUXTR ;--------------------------------------------------------------- ;! extracts text files from Q,U cubes for input to TARS ;# TASK ANALYSIS POLARIZATION ;----------------------------------------------------------------------- ;; Copyright (C) 2012 ;; 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 ;----------------------------------------------------------------------- QUXTR LLLLLLLLLLLLUUUUUUUUUUUU CCCCCCCCCCCCCCCCCCCCCCCCCCCCC QUXTR Extract Q, U spectra to text files for TARS use INNAME Input I image name (name). INCLASS Input I image name (class). INSEQ 0.0 9999.0 Input I image name (seq. #). INDISK 0.0 9.0 Input I image disk unit #. IN2NAME Input U image name (name). IN2CLASS Input U image name (class). IN2SEQ 0.0 9999.0 Input U image name (seq. #). IN2DISK 0.0 9.0 Input U image disk unit #. OUTFILE Output text file base name VPARM 0.0 Ra,Dec pixel pairs to do ---------------------------------------------------------------- QUXTR Type: TASK Use: This task is used to extract Q/U spectra in text files for input to the TARS task which tests Faraday rotation synthesis. The Q and U images may be in any transposition, but freq-Ra-Dec works best. Adverbs: INNAME.....Input Q image name (name). No default. INCLASS....Input Q image name (class). Standard defaults. INSEQ......Input Q image name (seq. #). 0 => highest. INDISK.....Disk drive # of input Q image. 0 => any. IN2NAME....Input U image name (name). No default. IN2CLASS...Input U image name (class). Standard defaults. IN2SEQ.....Input U image name (seq. #). 0 => highest. IN2DISK....Disk drive # of input U image. 0 => any. OUTFILE....Text file base name for output spectra (numbers 1,2,3,.. will be appended). VPARM......Up to 15 pairs of the Ra,Dec pixel numbers to be written the text file(s). A zero terminates the list. ------------------------------------------------------------------------