; XYRATIO ;--------------------------------------------------------------- ;! Ratio of X to Y units per pixel ;# ADVERB 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 ;----------------------------------------------------------------------- ;--------------------------------------------------------------- XYRATIO LLLLLLLLLLLLUUUUUUUUUUUU CCCCCCCCCCCCCCCCCCCCCCCCCCCCC ---------------------------------------------------------------- XYRATIO Type: Adverb (Real) Use: The ratio in coordinate units per pixel separation along the X axis with respect to the Y axis. Null value: 0 Null value assignment is usually calculated from the pixel separations (X to Y increment) given in the image header if the axes are related (i.e. LL-MM). If the axes are unrelated (i.e. V-LL), the ratio of the Y to X windows is used (to give square plot). Some tasks set 0 to 1.4 in such cases. With DOTV true, the latter case is set to fill one of the two TV dimensions. Tasks: ALVAR.........Plots the Allan Variance statistic of a UV data set. ANBPL.........Plots and prints uv data converted to antenna based values. BLPLT.........Plots BLCAL tables in 2 dimensions as function of baseline and IF. BLSUM.........Sums images over irregular sub-images, displays spectra. BPEPL.........Plots bandpass tables overlaying multiple times like BPEDT. BPLOT.........Plots bandpass tables in 2 dimensions as function of time. BSTST.........Graphical display of solutions to frequency-switched data. CAPLT.........Plots closure amplitude and model from CC file. CCNTR.........Generate a contour plot file from an image with CC or MF plotted. CLPLT.........Plots closure phase and model from CC file. CNTR..........Generate a contour plot file or TV plot from an image. FGPLT.........Plots selected contents of FG table. GREYS.........Plots images as contours over multi-level grey. ISPEC.........Plots and prints spectrum of region of a cube. KNTR..........Make a contour/grey plot file from an image w multiple panels. PCHIS.........Generates a histogram plot file from text input, e.g. from PCRMS. PCNTR.........Generate plot file with contours plus polarization vectors. PCPLT.........Plots pulse-cal tables in 2 dimensions as function of time. PDPLT.........Plots selected contents of PD tables. PEEK..........Fits pointing model function to output from the VLA. PFPL1.........Paraform Task to generate a plot file: (does grey scale). PLOTC.........Plots color schems used by 3-color plot tasks. PLOTR.........Basic task to generate a plot file from text input. POSSM.........Task to plot total and cross-power spectra. PROFL.........Generates plot file for a profile display. PRTAN.........Prints the contents of the ANtenna extension file. RFLAG.........Flags data set based on time and freq rms in fringe visibilities. RM2PL.........Plots spectrum of a pixel with RMFIT fit. RSPEC.........Plots and prints spectrum of rms of a cube. SNBLP.........Plots selected contents of SN or CL files on a baseline basis. SNPLT.........Plots selected contents of SN, SY, TY, PC or CL files versus time. SYVSN.........Plots selected SY/TY data with SN solution values versus time. TARPL.........Plot input and output text files of the TARS task. UVHOL.........Prints holography data from a UV data base with calibration. UVPLT.........Plots data from a UV data base in multiple ways. VPLOT.........Plots uv data and model from CC file. XG2PL.........Plots spectrum of a pixel with XGAUS/AGAUS and ZEMAN/ZAMAN fits. ----------------------------------------------------------------