; XPARM ;--------------------------------------------------------------- ;! General adverb for up to 10 parameters, may refer to X coord ;# ADVERB GENERAL COORDINATES ;----------------------------------------------------------------------- ;; 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 ;----------------------------------------------------------------------- ;--------------------------------------------------------------- XPARM LLLLLLLLLLLLUUUUUUUUUUUU CCCCCCCCCCCCCCCCCCCCCCCCCCCCC ---------------------------------------------------------------- XPARM Type: Adverb (Real(10)) Use: A general adverb which contains ten elements as parameters to some process. When used with YPARM XPARM refers to the X-coordinate. It is used almost exclusively for the parameters of the gridding convolution function specified by XTYPE. Null value: Usually 0. See help files UVnTYPE for n = 1 to 6. Procedures: CXPOLN........Procedure to make complex polarization images and beam. LINIMAGE......Build image cube from multi-IF data set. Tasks: ACFIT.........Determine antenna gains from autocorrelations. XPARM is misused to list Rpol Tsys(IF). BSGEO.........Beam-switched Az-El image to RA-Dec image translation. BSGRD.........Task to image beam-switched single-dish data. CONFI.........Optimize array configuration by minimum side lobes. XPARM provides selection parameters for the mask image. CONPL.........Plots AIPS gridding convolution functions. HOLGR.........Read & process holography visibility data to telescope images. XPARM provides correcgtion and threshold parameters. IMAGR.........Wide-field and/or wide-frequency Cleaning / imaging task. SCIMG.........Full-featured imaging plus self-calibration loop with editing. SCMAP.........Imaging plus self-calibration loop with editing. SDGRD.........Task to select and image random-position single-dish data. SDIMG.........Task to select and image random-position single-dish data. UVIMG.........Grid UV data into an "image". UVMAP.........Makes images from calibrated UV data. ----------------------------------------------------------------