; IN4SEQ ;--------------------------------------------------------------- ;! specifies the sequence # of the 4th input image or data base ;# ADVERB CATALOG ;----------------------------------------------------------------------- ;; 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 ;----------------------------------------------------------------------- ;--------------------------------------------------------------- IN4SEQ LLLLLLLLLLLLUUUUUUUUUUUU CCCCCCCCCCCCCCCCCCCCCCCCCCCCC ---------------------------------------------------------------- IN4SEQ Type: Adverb (Real) Use: Data files are stored in AIPS under logical names which have 4 parts: a 12-character "name" field, a 6-character "class" field, and a numeric "sequence number" field. IN4SEQ is used to specify the "sequence number" field for the 4th of the input data files used by a verb or task. It is used as an integer number between 0 and 9999. Null value: 0 Null value means take the image having the highest sequence number which is consistent with the other adverb name parameters unless explicitly stated otherwise in the Help file for the verb or task. Verbs: CLR4NAME....Clears adverbs specifying the fourth input image GET4NAME....Fills 4th input image name parameters by catalog slot number. IM4HEAD.....Displays the image 4 header contents to terminal, message file. Q4HEADER....Verb to summarize the image 4 header: positions at center. Tasks: COMB........Combines two images by a variety of mathematical methods. The 4th image is of noise for the 2nd image. GREYS.......Plots images as contours over multi-level grey. The 4th image is for color blue. IMAGR.......Wide-field and/or wide-frequency Cleaning / imaging task. The 4th image is of spectral curvature. KNTR........Make a contour/grey plot file from an image w multiple panels. The 4th image is of polarization angle or U. MEDI........Combines four images by a variety of mathematical methods. OOSUB.......Subtracts/divides a model from/into a uv data base. The 4th image is of spectral curvature. PCNTR.......Generate plot file with contours plus polarization vectors. The 4th image may be used for contours or grey scale. PDPLT.......Plots selected contents of PD tables. RMFIT.......Fits 1-dimensional polarization spectrum to Q/U cube. The 4th image is from FARS, either the phase or the imaginary part. TVSPC.......Display images and spectra from a cube interactively. The 4th image is an optional XYf cube to be displayed one f at a time. VBGLU.......Glues together data from multiple passes thru the VLBA correlator. WTSUM.......Task to do a a sum of images weighted by other images. The 4th image is of weights assigned to the 2nd image. Procedures: IMFRING.....Large image delay fitting with IM2CC and OOFRING. The 4th image is of spectral curvature. IMSCAL......Large image self-cal with IM2CC and OOCAL. The 4th image is of spectral curvature. LINIMAGE....Build image cube from multi-IF data set. The 4th image is of spectral curvature. OOCAL.......Determines antenna complex gain with frequency-dependent models. The 4th image is of spectral curvature. OOFRING.....Fringe fit data to determine calibration with spectral index options. The 4th image is of spectral curvature. ----------------------------------------------------------------