; CMODEL ;--------------------------------------------------------------- ;! specifies the method by which the uv model is computed ;# ADVERB IMAGING MODELING UV CALIBRATION ;----------------------------------------------------------------------- ;; Copyright (C) 1995 ;; 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 ;----------------------------------------------------------------------- CMODEL LLLLLLLLLLLLUUUUUUUUUUUU CCCCCCCCCCCCCCCCCCCCCCCCCCCCC ---------------------------------------------------------------- CMODEL Type: Adverb (String*4) Use: To select the source of the model used to compute the fringe visibilities of the source model. 'COMP' uses a Clean components table 'IMAG' uses an image. ' ' uses COMP if a CC file is present, else IMAG. Null value: ' ' => task chooses Tasks: CALIB.......Determines the calibration to be applied to a uv data set given a model of the source. UVSUB.......Subtracts/divides a model from/into a uv data base. ----------------------------------------------------------------