; IN3NAME ;--------------------------------------------------------------- ;! specifies the "name" of the 3rd 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 ;----------------------------------------------------------------------- ;--------------------------------------------------------------- IN3NAME LLLLLLLLLLLLUUUUUUUUUUUU CCCCCCCCCCCCCCCCCCCCCCCCCCCCC ---------------------------------------------------------------- IN3NAME Type: Adverb (String*12) Use: Data files are stored in AIPS under logical names which have 3 parts: a 12-character "name" field, a 6-character "class" field, and a numeric "sequence number" field. IN3NAME is used to specify the "name" field for the 3rd of the input data files used by a verb or task. This adverb is handled by AIPS tasks and verbs under special "wildcard" rules. These rules determine which test strings (e.g. image names in the catalog) match the user-specified string. Except for '*', '?', and trailing blanks (when an * is present), all characters specified in IN3NAME must exactly match the corresponding characters in the test string. A '?' in IN3NAME matches any single character in the test string. An '*' in IN3NAME matches 0 or more characters in the test string. Thus, IN3NAME = '*' matches any test string. IN3NAME = 'A?B*D' matches 'ASBD', 'A BXYZD D', and 'A3B45678901D', but does not match 'ABCD' or 'ASBCDE'. Null value: ' ' Taken as '*' unless the Help file for the specific task or verb states otherwise. Verbs: CLR3NAME......Clears adverbs specifying the third input image. GET3NAME......Fills 3rd input image name parameters by catalog slot number. IM3HEAD.......Displays the image 3 header contents to terminal, message file. Q3HEADER......Verb to summarize the image 3 header: positions at center. Procedures: IMFRING.......Large image delay fitting with IM2CC and OOFRING. The 3rd image is of spectral index. IMSCAL........Large image self-cal with IM2CC and OOCAL. The 3rd image is of spectral index. LINIMAGE......Build image cube from multi-IF data set. The 3rd image is of spectral index. OOCAL.........Determines antenna complex gain with frequency-dependent models. The 3rd image is of spectral index. OOFRING.......Fringe fit data to determine calibration with spectral index options. The 3rd image is of spectral index. Tasks: BPASS.........Computes spectral bandpass correction table. The 3rd data set is the "channel 0" data. COMB..........Combines two images by a variety of mathematical methods. The third image is of noise corresponding to the 1st image. CPASS.........Computes polynomial spectral bandpass correction table. The 3rd data set is the "channel 0" data. GREYS.........Plots images as contours over multi-level grey. The 3rd image is in the green coor. IBLED.........Interactive BaseLine based visibility EDitor. The 3rd image is a Clean model. IMAGR.........Wide-field and/or wide-frequency Cleaning / imaging task. The 3rd image is of spectral index. IMLHS.........Converts images to luminosity/hue TV display. The 3rd image is of saturation. KNTR..........Make a contour/grey plot file from an image w multiple panels. The 3rd image is of Q or total polarization. MEDI..........Combines four images by a variety of mathematical methods. MODIM.........Adds images of model objects to image cubes in IQU polarization. the 3rd image is of U polarization. OOSUB.........Subtracts/divides a model from/into a uv data base. The 3rd image is of spectral index. PCNTR.........Generate plot file with contours plus polarization vectors. The 3rd image is of polarization angle. PDPLT.........Plots selected contents of PD tables. QUFIX.........Determines Right minus Left phase difference, corrects cal files. The 3rd image is of calibrated spectral polarization that is lacking the RLDIF correction. RFARS.........Correct Q/U cubes for Faraday rotation synthesis results. The 3rd image os of rotation measure. RMFIT.........Fits 1-dimensional polarization spectrum to Q/U cube. The 3rd image is of unpolarized intensity (Stokes I). SPCOR.........Task to correct an image for a primary beam and spectral index. the 3rd image is of spectral curvature. TVHUI.........Make TV image from images of intensity, hue, saturation. The 3rd image is of saturation. TVRGB.........Make TV image from images of true color (RGB) images. The 3rd image is of blue (if needed). TVSPC.........Display images and spectra from a cube. The 3rd image is of a second optional transposed cube. UTESS.........Deconvolves images by maximizing emptiness. The 3rd image is of default levels. VBGLU.........Glues together data from multiple passes thru the VLBA corr. VTESS.........Deconvolves sets of images by the Maximum Entropy Method. The 3rd image is of default levels. WTSUM.........Task to do a a sum of images weighted by other images. The 3rd image is of weights corresponding to the 1st image. ----------------------------------------------------------------