; SPECR ;--------------------------------------------------------------- ;! Spectral regridding task for UV data ;# TASK UV IMAGING ;----------------------------------------------------------------------- ;; Copyright (C) 1995-1996, 2008 ;; 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 ;----------------------------------------------------------------------- SPECR LLLLLLLLLLLLUUUUUUUUUUUU CCCCCCCCCCCCCCCCCCCCCCCCCCCCC SPECR: Spectral regridding task for uv data INNAME Input UV data (name) INCLASS Input UV data (class) INSEQ Input UV data (seq. #) INDISK Input UV data disk # OUTNAME Output uvdata name (name) OUTCLASS Output uv data class OUTDISK Output uvdata disk # OUTSEQ -1.0 32000.0 Output seq. no. NPOINTS 2.0 8192.0 # channels in output data BADDISK Disk #'s to avoid ---------------------------------------------------------------- SPECR Type: Task Use: Spectral regridding of UV line data. The user specifies the number of channels required in the output database and SPECR will regird the data to obtain that spectral resolution. It can either increase or decrease the spectral resolution. Some care must be taken by the user to avoid totally over-sampling the spectra. Output is compressed if input is compressed. NOTE: this task does NOT apply flagging or calibration tables to the input UV data. Run SPLIT first if that operation is desired. Adverbs: INNAME.....Input UV data file (name). Standard defaults. INCLASS....Input UV data file (class). Standard defaults. INSEQ......Input UV data file (seq. #). 0 => highest. INDISK.....Input UV data file disk #. 0 => any. OUTNAME....Output UV data name (name). Standard defaults. OUTCLASS...Output UV data file (class). OUTDISK....The disk # of output data. 0 => highest with space. OUTSEQ.....Output sequence number. 0 => new file. NPOINTS....The number of spectral channels (per IF and polarization) required in the output data file. BADDISK....Disk #'s to avoid for scratch files ----------------------------------------------------------------