; MATCH ;--------------------------------------------------------------- ;! changes antenna, source, FQ numbers to match a data set ;# Task UV VLBI ;----------------------------------------------------------------------- ;; Copyright (C) 2000-2001, 2005 ;; 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 ;----------------------------------------------------------------------- MATCH LLLLLLLLLLLLUUUUUUUUUUUU CCCCCCCCCCCCCCCCCCCCCCCCCCCCC MATCH Task to modify source, antenna, FQ numbers to match INNAME Input UV file name (name) INCLASS Input UV file name (class) INSEQ 0.0 9999.0 Input UV file name (seq. #) INDISK 0.0 9.0 Input UV file disk unit # IN2NAME Master UV file name. IN2CLASS Master UV file class. IN2SEQ 0.0 9999.0 Master UV file seq. # IN2DISK 0.0 9.0 Master UV file volumn number OUTNAME Output UV file name (name) OUTCLASS Output UV file name (class) OUTSEQ -1.0 9999.0 Output UV file name (seq. #) OUTDISK 0.0 9.0 Output UV file disk unit #. DOALL 0.0 7.0 Do antenna, source, frequency flags ---------------------------------------------------------------- MATCH Task: This task will make the antenna, source, and FQ numbers of the input data set match those of a master data set. The two data sets must be very similar or this will not work. A need for this can arise from various VLBA correlators that correlate only a portion of the data at any one pass or output tape file and number the antennas, sources, and FQs independently in each pass. The output AN file(s) will contain all antennas from both input files (of matching subarray number) suitably renumbered. FQ and SU tables are handled similarly. Adverbs: INNAME.....Input UV file name (name). Standard defaults. INCLASS....Input UV file name (class). Standard defaults. INSEQ......Input UV file name (seq. #). 0 => highest. INDISK.....Disk drive # of input UV file. 0 => any. IN2NAME....Master UV file name. IN2CLASS...Master UV file class. IN2SEQ.....Master UV file sequence number. IN2DISK....Master UV file sequence number. OUTNAME....Output UV file name (name). Standard defaults. OUTCLASS...Output UV file name (class). Standard defaults. OUTSEQ.....Output UV file name (seq. #). 0 => highest unique OUTDISK....Disk drive # of output UV file. 0 => highest with space for the file. DOALL......Binary flags: value 1 => do antennas, 2 => do sources, 4 => do frequencies. So 7 => do all 3. <= 0 => 7. For VBGLU usage, the files can have only one FREQID and must differ in frequency, so set DOALL=3. ----------------------------------------------------------------