; CMODEL ;--------------------------------------------------------------- ;! specifies the method by which the uv model is computed ;# ADVERB IMAGING MODELING UV CALIBRATION ;----------------------------------------------------------------------- ;; Copyright (C) 1995, 2020 ;; 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: BLCAL......Compute closure offset corrections. BLCHN......Compute closure offset corrections on a channel-by-channel basis. BLING......Find residual rate and delay on individual baselines. BPASS......Computes spectral bandpass correction table. CALIB......Determines the calibration to be applied to a uv data set given a model of the source. CPASS......Computes polynomial spectral bandpass correction table. FRING......Fringe fit data to determine antenna calibration, delay, rate. KRING......Fringe fit data to determine antenna calibration, delay, rate. LPCAL......Determines instrumental polarization for UV data, OOSUB......Subtracts/divides a model from/into a uv data base. PCAL.......Determines instrumental polarization for UV data. RLCAL......Determines instrumental right-left phase versus time (a self-cal). UVCON......Generate sample UV coverage given a user defined array layout. UVSUB......Subtracts/divides a model from/into a uv data base. Procedures: OOCAL......Determines antenna complex gain with frequency-dependent models. OOFRING....Fringe fit data to determine calibration with spectral index options. VLBABPSS...Computes spectral bandpass correction table. ----------------------------------------------------------------