; VLBI ;--------------------------------------------------------------- ;! Information about VLBI ;# INFORMATION GENERAL ;----------------------------------------------------------------------- ;; Copyright (C) 1995-1998, 2000-2003 ;; 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 ;----------------------------------------------------------------------- ;--------------------------------------------------------------- VLBI LLLLLLLLLLLLUUUUUUUUUUUU CCCCCCCCCCCCCCCCCCCCCCCCCCCCC ---------------------------------------------------------------- List of verbs, adverbs, tasks in category VLBI ACCOR Corrects cross amplitudes using auto correlation measurements ACFIT Determine antenna gains from autocorrelations AFILE sorts and edits MkIII correlator A-file. ALIAS adverb to alias antenna numbers to one another ANCAL Places antenna-based Tsys and gain corrections in CL table ANTAB Read amplitude calibration information into AIPS APCAL Apply TY and GC tables to generate an SN table BANDPOL specifies polarizations of individual IFs BLING find residual rate and delay on individual baselines BSPRT print BS tables CL2HF Convert CL table to HF table CLCOR applies user-selected corrections to the calibration CL table CLPLT plots closure phase and model from CC file CROSSPOL Procedure to make complex poln. images and beam. CRSFRING Procedure to calibrate cross pol. delay and phase offsets CVEL shifts spectral-line UV data to a given velocity CXPOLN Procedure to make complex poln. images and beam. DFCOR applies user-selected corrections to the calibration CL table DTSIM Generate fake UV data EDITR Interactive baseline-oriented visibility editor using the TV FRING fringe fit data to determine antenna calibration, delay, rate FRMAP Task to build a map using fringe rate spectra FRPLT Task to plot fringe rate spectra FXAVG Procedure to enable VLBA delay de-correlation corrections FXPOL Corrects VLBA polarization assignments HF2SV convert HF tables from FRING/MBDLY to form used by Calc/Solve HFPRT write HF tables from CL2HF HLPIBLED Interactive Baseline based visibility Editor - internal help HLPSCIMG Cleaning tasks - internal help HLPSCMAP Cleaning tasks - internal help HYB RUN to set parameters for HYBRID (CALIB/MX) self-cal imaging IBLED Interactive BaseLine based visibility EDitor KRING fringe fit data to determine antenna calibration, delay, rate M3TAR translate Haystack MKIII VLBI format "A" TAR's into AIPS MATCH changes antenna, source, FQ numbers to match a data set MBDLY Fits multiband delays from IF phases, updates SN table MERGECAL Procedure to merge calibration records after concatenation MK3IN translate Haystack MKIII VLBI format "A" tapes into AIPS MK3TX extract text files from a MKIII VLBI archive tape OBPLT Plot columns of an OB table. PCCOR Corrects phases using PCAL tones data from PC table PCLOD Reads ascii file containing pulse-cal info to PC table. PHSLIMIT gives a phase value in degrees POLSN Make a SN table from cross polarized fringe fit RESEQ Resequence antennas SNEDT Interactive SN/CL table editor using the TV TECOR Calculate ionospheric delay and Faraday rotation corrections TFILE sorts and edits MkIII correlator UNIX-based A-file. UVPOL modifies UV data to make complex image and beam VBCAL Scale visibility amplitudes by antenna based constants VBGLU Glues together data from multiple passes thru the VLBA corr. VBMRG Merge VLBI data, eliminate duplicate correlations VLASUMM Plots selected contents of SN or CL files VLBACALA applies a-priori amplitude corrections to VLBA data VLBACPOL Procedure to calibrate cross-polarization delays VLBACRPL Plots crosscorrelations VLBAFIX looks for subarrays in VLBA data VLBAFPOL checks polarization labels for VLBA data VLBAFQS Copies different FQIDS to separate files VLBAFRGP fringe fit data to determine antenna calibration, delay, rate VLBAFRNG fringe fit data to determine antenna calibration, delay, rate VLBA Procedure to read and process VLBA data (Phil Diamond) VLBAKRGP fringe fit data to determine antenna calibration, delay, rate VLBAKRNG fringe fit data to determine antenna calibration, delay, rate VLBALOAD loads VLBA data VLBAMCAL merges redundant calibration data VLBAMPCL loads VLBA data VLBAPANG Corrects for parallactic angle VLBAPCOR loads VLBA data VLBAPIPE applies amplitude and phase calibration procs to VLBA data VLBASNPL Plots selected contents of SN or CL files VLBASRT looks for subarrays in VLBA data VLBASUBS looks for subarrays in VLBA data VLBASUMM Plots selected contents of SN or CL files VLBAUTIL Procedures to simplify the reduction of VLBA data VLBIN Task to read VLBI data from an NRAO/MPI MkII correlator VLOG Pre-process external VLBA calibration files VPLOT plots uv data and model from CC file (the fast version ov VBPLT)