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13.41 VLA

ALBUS    Calculate ionospheric delay and Faraday rotation using ALBUS
APGPS    Apply GPS-derived ionospheric corrections
ASDMFILE    Full path to EVLA ASDM/BDF directory
BDF2AIPS    Read EVLA ASDM/BDF data into AIPS
BDFLIST    List contents of EVLA ASD data file
BPWAY    Determines channel-dependent relative weights
BREAK    procedure to TELL FILLM to break all current uv files, start new
CALDIR    lists calibrator source models available as AIPS FITS files
CALIN    specifies name of input disk file usually with calibration data
CLCOR    applies user-selected corrections to the calibration CL table
CONFIG    Configuration ID number within an EVLA ASDM/BDF data set
CVEL    shifts spectral-line UV data to a given velocity
DAYFX    Fixes day number problems left by FILLM
DFCOR    Applies ATMO differential corrections to the calibration CL table
DOOSRO    calibrating amplitude and phase, and imaging VLA data
DOVLAMP    Produces amp calibration file for phased-VLA VLBI data
FARAD    add ionospheric Faraday rotation to CL table
FEW    procedure to TELL FILLM to append incoming data to existing uv files
FILLM    reads VLA on-line/archive format uv data tapes (post Jan 88)
FIXAL    least squares fit aliasing function and remove
FLOPM    reverses the spectral order of UV data, can fix VLA error
FRMAP    Task to build a map using fringe rate spectra
FXALIAS    least squares fit aliasing function and remove
GCPLT    Plots gain curves from text files
GPSDL    Calculate ionospheric delay and Faraday rotation corrections
LDGPS    load GPS data from an ASCII file
MANY    procedure to TELL FILLM to start new uv files on each scan
MAPBM    Map VLA beam polarization
MORIF    Combines IFs or breaks spectral windows into multiple windows (IFs)
NCHAN    Number of spectral channels in each spectral window
NIF    Number of IFs (spectral windows) in a data set
PANEL    Convert HOLOG output to panel adjustment table
PCVEL    shifts spectral-line UV data to a given velocity: planet version
PEEK    fits pointing model function to output from the VLA
PIPEAIPS    calibrating amplitude and phase, and imaging VLA data
PRTSY    Task to print statistics from the SY table
QUIT    procedure to TELL FILLM to stop at the end of the current scan
REIFS    Breaks spectral windows into multiple spectral windows (IFs)
REWAY    computes weights based in rms in spectra
RFLAG    Flags data set based on time and freq rms in fringe visibilities
STOP    procedure to TELL FILLM to break all current uv files and stop
SYHIS    Task to clip, filter, smooth SY tables and plot histograms
SYPRT    Task to print values from the SY table
SYSOL    undoes and re-does nominal sensitivity application for Solar data
TECOR    Calculate ionospheric delay and Faraday rotation corrections
TELFLM    procedure to TELL real-time FILLM a new APARM(1) value
TLCAL    Converts JVLA telcal files to an SN file
TYAPL    undoes and re-does nominal sensitivity application
TYSMO    smooths and filters a calibration TY or SY table
USERLIST    Alphabetic and numeric list of VLA users, points to real list
VLABP    VLA antenna beam polarization correction for snapshot images
VLAMP    Makes ANTAB file for phased VLA used in VLBI observations
VLANT    applies VLA/EVLA antenna position corrections from OPs files
VLAPROCS    Procedures to simplify the reduction of VLBA data
VLARUN    Calibrating amplitude and phase, and imaging VLA data
VLATECR    Calculate ionospheric delay and Faraday rotation corrections

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