As of Wed Jan 17 7:31:20 2018

UVHOL: Prints/writes holography data with calibration


INNAME                             Input UV file name (name)
INCLASS                            Input UV file name (class)
INSEQ             0.0     9999.0   Input UV file name (seq. #)
INDISK                             Input UV file disk unit #
SOURCES                            Sources to print, ' '=>all.
QUAL            -10.0              Qualifier -1=>all
CALCODE                            Calibrator code '    '=>all
STOKES                             'FULL' in HOLG for 4 output
                                   files, 'IQUV', 'IV' also
SELBAND                            Bandwidth to select (kHz)
SELFREQ                            Frequency to select (MHz)
FREQID                             Freq. ID to select.
TIMERANG                           Time range to select
ANTENNAS                           Antennas to print
BASELINE                           Baselines with ANTENNAS
SUBARRAY          0.0     1000.0   Subarray, 0 => 1
ICHANSEL          0.0     4096.0   Spectral channels to average
BIF                                IF number to print
DOCALIB          -1.0      101.0   > 0 calibrate data & weights
                                   > 99 do NOT calibrate weights
GAINUSE                            CAL (CL or SN) table to apply
DOPOL            -1.0       10.0   If >0 correct polarization.
PDVER                              PD table to apply (DOPOL>0)
BLVER                              BL table to apply.
FLAGVER                            Flag table version
DOBAND           -1.0       10.0   If >0 apply bandpass cal.
                                   Method used depends on value
                                   of DOBAND (see HELP file).
BPVER                              Bandpass table version
SMOOTH                             Smoothing function. See
                                   HELP SMOOTH for details.
NCOUNT            0.0   30000.0    # of sample. 0 => 1 page.
WTUV              0.0    1000.0    Scale UV (actually LM) by
                                   WTUV, 0 => 1 in HOLG, else
                                   0 => 1000
OPTYPE                             Choice of format type:
                                   'HOLG' write holography file
                                   else   print holography data
NPOINTS           0.0    1000.0    Number of samples to keep
                                   at the end of each pointing
                                   Used if APARM(1) = 0
                                   0 => 100
APARM                              (1) 0 => NPOINTS used
                                       1 => APARM(2,3) used
                                   (2) number of samples dropped
                                       at the beginning of
                                       each pointing
                                   (3) number of samples dropped
                                       at the end of
                                       each pointing
                                   (4) > 0  write elevation and
                                      azimuth at beg/end of scan
                                   (5) > 0 => average data over
                                      reference antennas
                                   (6) > 0 => average each
                                      pointing over time
                                   (7) > 0 => display amp/phase
                                      in 'HOLG'
                                   (8) > 0 => average data over
                                      moving antennas
                                   (9) > 0 => scalar amplitudes
                                      in time & antenna average
                                   (10) > 0 -> apply parallactic
                                      angle correction on DOPOL
BDROP             0.0    1000.0    Minimum number of samples to
                                   keep the pointing at all
DPARM                              1 : <0 => Range of (U,V,W),
                                       amplitude and weight is
                                       determined automatically;
                                       >= 0 => Ranges are fixed
                                       minimize the run time.
                                   2 : Maximum weight; 0 => 99.0
                                   3 : Minimum weight; 0 => 0.11
                                   4 : Maximum amplitude; 0=>9.9
                                   5 : Maximum of ABS(U),ABS(V),
                                       ABS(W) in klambda;
                                       0 => 10000
DOCRT            -3.0     132.0    > 0 -> use the terminal,
                                   else use the line printer
                                   > 72 => terminal width
                                   Printer disk file to save
                                   HOLG: area to write outputs
BADDISK                            Disk to avoid for scratch.


Type: Task
Use:  Prints holography data from a u,v data base, optionally making
      retained text files.  UVHOL is similar to UVPRT, but does only
      the special holography modes which used to be a part of UVPRT.
      These include printing for display purposes and the ability to
      write files for input to HOLGR.
  INNAME.....Input UV file name (name)    Standard defaults.
  INCLASS....Input UV file name (class)   Standard defaults.
  INSEQ......Input UV file name (seq. #)  0 => highest.
  INDISK.....Disk drive # of input UV file.  0 => any.
  SOURCES....List of sources to be printed. '  '=> all; if any
             starts with a '-' then all except ANY source named.
  QUAL.......Qualifier of source to be printed.    -1 => all.
  CALCODE....Calibrator code of sources to print.  ' '=> all.
  STOKES.....The usual Stokes parameter.  In HOLG mode, FULL means to
             write all 4 polarizations to disk files, IQUV means to
             write all 4 Stokes polarizations, IV means to write the
             two parallel hand Stokes, otherwise RR and LL only are
             written.  When simply printing, STOKES beginning with I
             means 'IQUV', otherwise FULL is used.  If fewer than 4
             Stokes are available, the task now takes appropriate
             action in the STOKES adverb.
  SELBAND....Bandwidth of data to be selected. If more than one IF is
             present SELBAND is the width of the first IF required.
             Units = kHz. For data which contain multiple
             bandwidths/frequencies the task will insist that some form
             of selection be made by frequency or bandwidth.
  SELFREQ....Frequency of data to be selected. If more than one IF is
             present SELFREQ is the frequency of the first IF required.
             Units = MHz.
  FREQID.....Frequency identifier to select (you may determine which is
             applicable from the OPTYPE='SCAN' listing produced by
             LISTR). If either SELBAND or SELFREQ are set, their values
             overide that of FREQID.  However, setting SELBAND and
             SELFREQ may result in an ambiguity.  In that case, the task
             will request that you use FREQID.  If all SELBAND, SELFREQ
             and FREQID are not specified (.le. 0) then all FQ ids will
             be selected.
  TIMERANG...Time range of the data to be printed. In order: Start day,
             hour, min. sec, end day, hour, min. sec. Days relative to
             reference date.
  ANTENNAS...A list of the reference antennas to print.  At least one
             must be given.  The first is used to name the output file
             in HOLG mode.
  BASELINE...A list of the moving antennas.  At least one must be
  SUBARRAY...Subarray number to print.       0 => 1.
  ICHANSEL.. Array of start, stop, and increment channel numbers plus
             an IF used for channel selection in the averaging to
             compute data displayed.  Up to 20 sets of channels/IF may
             be entered.  The first having ICHANSEL(2,i) <= 0
             terminates the list.  ICHANSEL(4,i) is the IF number,
             with <= 0 meaning all IFs.  If an IF has no ICHANSEL set
             for it, then the inner 75 percent of that IF is used.  Note
             that only the values for IF # = BIF are actually used.
  BIF........IF number to print.             0 => 1
  DOCALIB....If true (>0), calibrate the data using information in the
             specified Cal (CL) table for multi-source or SN table for
             single-source data.  Also calibrate the weights unless
             DOCALIB > 99 (use this for old non-physical weights).
  GAINUSE....Version number of the Cal. table to apply to the data if
             DOCALIB=1.  Refers to a CL table for multi-source data or
             an SN table for single source.   0 => highest.
  DOPOL......If > 0 then correct data for instrumental polarization as
             represented in the AN or PD table.  This correction is
             only useful if PCAL has been run or feed polarization
             parameters have been otherwise obtained.  See HELP DOPOL
             for available correction modes: 1 is normal, 2 and 3 are
             for VLBI.  1-3 use a PD table if available; 6, 7, 8 are
             the same but use the AN (continuum solution) even if a PD
             table is present.
  PDVER......PD table to apply if PCAL was run with SPECTRAL true and
             0 < DOPOL < 6.  <= 0 => highest.
  BLVER......Version number of the baseline based calibration (BL) table
             to apply. <0 => apply no BL table,   0 => highest.
  FLAGVER....Specifies the version of the flagging table to be applied.
             0 => highest numbered table.  <0 => no flagging to be
  DOBAND.....(multisource) If true (>0) then correct the data for the
             shape of the antenna bandpasses using the BP table
             specified by BPVER.  The correction has five modes:
             (a) if DOBAND=1 all entries for an antenna in the table
             are averaged together before correcting the data.
             (b) if DOBAND=2 the entry nearest in time (including
             solution weights) is used to correct the data.
             (c) if DOBAND=3 the table entries are interpolated in
             time (using solution weights) and the data are then
             (d) if DOBAND=4 the entry nearest in time (ignoring
             solution weights) is used to correct the data.
             (e) if DOBAND=5 the table entries are interpolated in
             time (ignoring solution weights) and the data are then
  BPVER......(multi-source) specifies the version of the BP table to be
             applied. 0 => highest numbered table.
  SMOOTH.....Specifies the type of spectral smoothing to be applied to
             a uv database . The default is not to apply any smoothing.
             The elements of SMOOTH are as follows:
             SMOOTH(1) = type of smoothing to apply: 0 => no smoothing
               To smooth before applying bandpass calibration
                 1 => Hanning, 2 => Gaussian, 3 => Boxcar, 4 => Sinc
               To smooth after applying bandpass calibration
                 5 => Hanning, 6 => Gaussian, 7 => Boxcar, 8 => Sinc
             SMOOTH(2) = the "diameter" of the function, i.e. width
               between first nulls of Hanning triangle and sinc
               function, FWHM of Gaussian, width of Boxcar. Defaults
               (if < 0.1) are 4, 2, 2 and 3 channels for SMOOTH(1) =
               1 - 4 and 5 - 8, resp.
             SMOOTH(3) = the diameter over which the convolving
               function has value - in channels.  Defaults: 1,3,1,4
               times SMOOTH(2) used when input SMOOTH(3) < net
  NCOUNT.....List NCOUNT data points (after all data selection has been
             applied).      0 => 1 page listed.
             UVHOL will list up to 30000 visibilities.  This limit does
             not apply to HOLG and applies on a per antenna-pair basis
             for HOLO.
             Be aware that UVHOL now goes through the data to be printed
             twice, once to determine the u-v-w, data, and weight ranges
             and the second time to print things.  Using NCOUNT to
             reduce the time required by the first pass helps when DOCRT
             is true.
  WTUV.......Scale the "U" and "V" (actually sin^(-1)(theta) - the
             offset angle) values.  For HOLO, 0 => 1000.
             For HOLG, < 0.1 and > 10.0 are changed to 1.0.
             NOTE: this scaling may be required for HOLG to undo
             scaling done when selecting an IF in AIPS tasks such as
             UVCOP.  All such tasks must scale u,v,w by the ratio of
             the old reference frequency to the new reference
             frequency.  This is correct for the calibration scans in
             the holography data set, but not for the actual
             holography scans.  Use WTUV to undo this scaling.
  OPTYPE.....OPeration code to change details of the format:
             'HOLG' => write holography data from one or more antenna
                       pairs to 2 or 4 files per pair for use in HOLGR.
                       (No normal printing is done.)
                       Each line has 6 numbers: u, v, real, imag,
                       uncertainty in real, and in imag
                       or u, v, amplitude, phase, uncerainty in amp
                       and in phase
                       uncertainties are those in the mean numbers
                       (i.e. divided by sqrt(N-1))
             otherwise => print only holography data from one or more
                       antenna pairs.
  NPOINTS....Retain the last NPOINTS samples from each pointing.  Note
             that pointings are indicated by the W term in the U,V,W
             triplet.  For holography, W = 40000+X where X is a counter
             referring to the pointing or dwell currently selected.  The
             first samples for each dwell are suspect since not all
             antennas have settled down.  This option allows you to
             select only the last NPOINTS samples.  0 -> 100 (the upper
  APARM......(1) 0 => option determined by NPOINTS is used
                 1 => option determined by APARM(2,3) is used
             (2) number of samples dropped at the beginning of
                 each pointing
             (3) number of samples dropped at the end of
                 each pointing
             (4) >0 write elevation and azimuth at begining and
                 end of scans (only for OPTYPE = 'HOLG')
             (5) > 0 => average each baseline between a moving antenna
                 reference antenna over all reference antennas
             (6) > 0 => average all retained samples for each
             (7) > 0 => display amplitude and phase, otherwise real
                 and imaginary (HOLG only, amp and phase printed on
                 other OPTYPEs)
             (8) > 0 => average each baseline with reference
                 antenna(s) of all moving antennas.
             (9) > 0 => vector average data over spectral channels but
                 then display scalar average amplitudes when averaging
                 over time, reference antennas, and/or moving
             (10) For antenna-based display one does not want to apply
                 the parallactic angle correction when applying the
                 polarization D terms.  To apply them, set APARM(10)>0
                 for displays in source coordinates.
  BDROP......If a pointing has fewer than BDROP samples, then drop it
             entirely.  No default - 0 and 1 mean keep all.   Note
             that this is the total number of samples, not those after
             application of APARM(2) and APARM(3) (or NPOINTS).
  DPARM......Range of (U,V,W), amplitude and weight:
         (1) : < 0 => Range of (U,V,W), amplitude and weight is
             determined  automatically; If the data are large, the
             time for required additional pass of the data to provide
             the scaling can be rather large. To eliminate this extra
             pass use DPARM(1)=0.
             >= 0 => The ranges are fixed to the following values:
         (2) : Maximum weight; 0 => 99.0
         (3) : Minimum weight; 0 => 0.11
         (4) : Maximum amplitude; 0=>9.9
         (5) : Maximum of ABS(U),ABS(V),ABS(W) in lambda times WTUV
              (normally klambda); 0 => 10000
  DOCRT......False (<= 0) use the line printer if OUTPRINT = ' '
                   else write named OUTPRINT file only.
                   When OUTPRINT is not blank, DOCRT=-2 suppresses the
                   page-feed character on page headers and DOCRT=-3
                   suppresses page headers and most other header
                   information (non-HOLG mode).  When OUTPRINT is
                   blank, the line printer will be used.  UVHOL now
                   counts the lines to be printed before printing any
                   and asks for permission to continue if the count >
             True  (> 0) use the terminal interactively.  The task will
                   use the actual terminal width as a display limit
                   unless 72 < DOCRT < width.  In that case, the display
                   limit will be DOCRT characters.  132 width is best.
  OUTPRINT...Disk file name in which to save the line printer output.
             ' ' => use scratch and print immediately for interactive
             jobs - batch jobs use OUTPRINT = 'PRTFIL:BATCHjjj.nnn'
             (jjj= job #, nnn = user #).  When OUTPRINT is not blank,
             multiple outputs are concatenated, and the file is not
             actually printed.
             For HOLG mode only, OUTPRINT may give the name of a
             logical area plus optional file name to which to write
             the HOLGR data files (e.g. OUTPR = 'MYAREA' or OUTPR =
             'MYAREA:xxx', where xxx can be anything and MYAREA is a
             logical area defined before starting AIPS in the usual
             way).  If OUTPRINT gives only a logical name, then the
             name HOLOnn-mmppii is used where nn is the reference
             antenna (BASELINE(j)), mm is the antenna (or 0 if
             multiple), pp are 2 letters giving the polarization, and
             ii id the IF.  If xxx is not blank, then the output name
             is xxx (any number of letters) with ppii concatenated.
             If OUTPRINT is blank, then the disk area where you were
             when you started AIPS is used.  If OUTPRINT = 'xxx', xxx
             will be taken to be a disk area environment name.
  BADDISK....Disk numbers to avoid for scratch files.  Scratch files may
             be created by the sorting routines if calibration or
             flagging is applied.


Special notes on holography data, in HOLO or HOLG modes:

(1) Any included data that does not have a W > 40000 is assumed to be
    calibrator data and is ignored.  The source qualifier of
    holography data must be at least 40000, that of calibrators must
    be less than 40000.
(2) The W term is expected to be 40000 + 256*subqualifier + mode,
    where mode is supposed to be > 0.  When mode is 0, the data are
    assumed to be taken during an antenna turn-around phase and are
(3) When printing in these modes, the 40000 and n*256 parts of W are