; CC2IM ;--------------------------------------------------------------- ;! Make model image from a CC file ;# TASK ANALYSIS CALIBRATION ;----------------------------------------------------------------------- ;; 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 ;----------------------------------------------------------------------- CC2IM LLLLLLLLLLLLUUUUUUUUUUUU CCCCCCCCCCCCCCCCCCCCCCCCCCCCC CC2IM Converts a CC file into a model image INNAME Input image name (name) INCLASS Input image name (class) INSEQ 0.0 9999.0 Input image name (seq. #) INDISK 0.0 9.0 Input image disk unit # OUTNAME Output image name (name) OUTCLASS Output image name (class) OUTSEQ -1.0 9999.0 Output image name (seq. #) OUTDISK 0.0 9.0 Output image disk unit #. INVERS 0.0 CC version number CELLSIZE 0.0 Output image cell size asec DOCENTER -1.0 1.0 > 0 force ref pixel to center of output image IMSIZE Minimum size of image ---------------------------------------------------------------- CC2IM Task: Task which converts a CC file into an image. All components that are not flagged are used. Use TABED, TAFLG, or other tasks to prepare CC files if it is needed to limit the components used her. The output image may be used in CALIB and friends as a model if you enter CMODEL = 'SUBI'. If you use DOCENTER > 0, CMODEL may be set to 'IMAG' or ' '. Adverbs: INNAME.....Input image name (name). Standard defaults. INCLASS....Input image name (class). Standard defaults. INSEQ......Input image name (seq. #). 0 => highest. INDISK.....Disk drive # of input image. 0 => any. OUTNAME....Output image name (name). Standard defaults. OUTCLASS...Output image name (class). Standard defaults. OUTSEQ.....Output image name (seq. #). 0 => highest unique. OUTDISK....Disk drive # of output image. 0 => highest disk number with sufficient space. INVERS.....CC file version number CELLSIZE...Size in arc seconds for output image. 0 -> input image cell size. DOCENTER...> 0 -> make the image even larger so that the reference pixel will be at the center of the image IMSIZE.....Minimum X, Y size in pixels of the image. Use this with DOCENTER true to make model images from each scale of a multi-scale Clean. Then one can add the models together. ----------------------------------------------------------------