; EDITING ;--------------------------------------------------------------- ;! Information about EDITING ;# INFORMATION GENERAL ;----------------------------------------------------------------------- ;; Copyright (C) 1995-2004, 2006-2008, 2010-2015 ;; 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 ;----------------------------------------------------------------------- EDITING LLLLLLLLLLLLUUUUUUUUUUUU CCCCCCCCCCCCCCCCCCCCCCCCCCCCC ---------------------------------------------------------------- List of verbs, adverbs, tasks in category EDITING ACLIP edits suto-corr data for amplitudes, phases, and weights out of range CLIP edits data based on amplitudes, phases, and weights out of range CROWDED allows a task to perform its function in a crowded fashion DEFLG edits data based on decorrelation over channels and time DOFLAG Controls closure cutoff in gain solutions and flagging DOPLOT Controls plotting of something DOROBUST Controls method of averaging - simple mean/rms or robust EDITA Interactive TV task to edit uv data based on TY/SY/SN/CL tables EDITR Interactive baseline-oriented visibility editor using the TV EXPERT specifies an user experience level or mode FGDIF Compares affect of 2 FG tables FINDR Find normal values for a uv data set FLAGR Edit data based on internal RMS, amplitudes, weights FLGIT flags data based on the rms of the spectrum FTFLG interactive flagging of UV data in channel-time using the TV HLPEDICL Interactive SN/CL table uv-data editor - internal help HLPEDISN Interactive SN/CL table (not UV) editor - internal help HLPEDISS Interactive SY table (not UV) editor - internal help HLPEDISY Interactive SY table uv-data editor - internal help HLPEDITS Interactive TY table (not UV) editor - internal help HLPEDITY Interactive TY table uv-data editor - internal help HLPEDIUV Interactive uv-data editor - internal help HLPFTFLG Interactive time-channel visibility Editor - internal help HLPWIPER WIPER run-time help file IBLED Interactive BaseLine based visibility EDitor NOISE estimates the noise in images, noise level cutoff OFLAG uses on-line flag table information to write a flag table OUTFGVER selects version of the flagging table to be written REFLG Attempts to compress a flag table RFI Look for RFI in uv data RFLAG Flags data set based on time and freq rms in fringe visibilities SCANLENG specify length of "scan" SCIMG Full-featured imaging plus self-calibration loop with editing SCMAP Imaging plus self-calibration loop with editing SCUTOFF noise level cutoff SDLSF least squares fit to channels and subtracts from SD uv data SNEDT Interactive SN/CL/TY/SY table editor using the TV SNFLG Writes flagging info based on the contents of SN files SPFLG interactive flagging of UV data in channel-TB using the TV TABED Task to edit tables TAFLG Flags data in a Table extension file TVFLG interactive flagging of UV data using the TV UVFLG Flags UV-data UVFND prints selected data from UV data set to search for problems UVLIN Fits and removes continuum visibility spectrum, also can flag UVLSD least squares fit to channels and divides the uv data. UVLSF least squares fit to channels and subtracts from uv data. UVMLN edits data based on the rms of the spectrum VPFLG Resets flagging to all or all corss-hand whenever some are flagged WETHR Plots selected contents of WX tables, flags data based on WX WIPER plots and edits data from a UV data base using the TV