Public Member Functions | |
def | __init__ |
def | result |
def | __call__ |
def | paramgui |
def | defaults |
def | check_params |
def | description |
def | itsdefault |
Public Attributes | |
parameters | |
Static Public Attributes | |
rkey | |
Handle globals or user over-ride of arguments. | |
i_am_a_casapy_task | |
list | retval |
This function sets the default values but also will return the list of parameters or the default value of a given parameter. | |
string | valornotval |
tuple | retval |
Private Attributes | |
__bases__ | |
__doc__ | |
__globals__ | |
Static Private Attributes | |
string | __name__ |
dictionary | __async__ |
Definition at line 18 of file pclean_cli.py.
def pclean_cli.pclean_cli_.__init__ | ( | self | ) |
Definition at line 26 of file pclean_cli.py.
def pclean_cli.pclean_cli_.__call__ | ( | self, | |
vis = None , |
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imagename = None , |
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imsize = None , |
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cell = None , |
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phasecenter = None , |
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stokes = None , |
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mask = None , |
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field = None , |
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spw = None , |
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ftmachine = None , |
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alg = None , |
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scales = None , |
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cyclefactor = None , |
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majorcycles = None , |
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niter = None , |
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gain = None , |
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threshold = None , |
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weighting = None , |
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robust = None , |
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npixels = None , |
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mode = None , |
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nterms = None , |
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start = None , |
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nchan = None , |
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width = None , |
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restfreq = None , |
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interactive = None , |
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npercycle = None , |
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wprojplanes = None , |
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facets = None , |
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overwrite = None , |
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uvtaper = None , |
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outertaper = None , |
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timerange = None , |
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uvrange = None , |
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antenna = None , |
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scan = None , |
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observation = None , |
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pbcor = None , |
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minpb = None , |
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clusterdef = None , |
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async = None |
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) |
Invert and deconvolve images with parallel engines Keyword arguments: Invert and deconvolve images with parallel engines Form images from visibilities. Handles continuum and spectral line cubes using module pcont and pcube respectively. vis -- Name of input visibility file default: none; example: vis='ngc5921.ms' imagename -- Pre-name of output CASA image. (only the prefix) default: none; example: imagename='m2', output images are: m2.image; cleaned and restored image With or without primary beam correction m2.psf; point-spread function (dirty beam) m2.model; image of clean components m2.mask; image containing clean regions, when interative=True imsize -- Image pixel size (x,y). DOES NOT HAVE TO BE A POWER OF 2 default: [256,256]; example: imsize=[350,350] imsize=500 is equivalent to imsize=[500, 500] Avoid odd-numbered imsize. cell -- Cell size (x,y) default: '1.0arcsec'; example: cell=['0.5arcsec', '0.5arcsec'] or cell=['1arcmin', '1arcmin'] cell='1arcsec' is equivalent to cell=['1arcsec', '1arcsec'] NOTE:cell=2.0 => cell=['2arcsec', '2arcsec'] phasecenter -- direction measure or fieldid for the mosaic center default: '' => first field selected; example: phasecenter=6 or phasecenter='J2000 19h30m00 -40d00m00' mask -- mask image to be used for CLEANing. As long as the image has the same shape (size), mask images from a previous interactive session can be used for a new execution. Only an image mask is allowed at this stage. Text formats not allowed yet. field -- Select fields in MS. Use field id(s) or field name(s). ['go listobs' to obtain the list id's or names] default: ''= all fields If field string is a non-negative integer, it is assumed to be a field index otherwise, it is assumed to be a field name examples: field='0~2'; field ids 0,1,2 field='0,4,5~7'; field ids 0,4,5,6,7 field='3C286,3C295'; field named 3C286 and 3C295 field = '3,4C*'; field id 3, all names starting with 4C spw --Select spectral window/channels NOTE: This selects the data passed as the INPUT to mode default: ''=all spectral windows and channels examples: spw='0~2,4'; spectral windows 0,1,2,4 (all channels) spw='0:5~61'; spw 0, channels 5 to 61 spw='< 2'; spectral windows less than 2 (i.e. 0,1) spw='0,10,3:3~45'; spw 0,10 all channels, spw 3, channels 3 to 45. spw='0~2:2~6'; spw 0,1,2 with channels 2 through 6 in each. spw='0:0~10;15~60'; spectral window 0 with channels 0-10,15-60 spw='0:0~10,1:20~30,2:1;2;3'; spw 0, channels 0-10, spw 1, channels 20-30, and spw 2, channels, 1,2 and 3 ftmachine -- Fourier Transform Engine (Gridding method) Options: 'ft' (standard interferometric gridding), 'sd' (standard single dish), 'mosaic' (grid using PB as convolution function). 'wproject' (wprojection gridder to correct for widefield 'w' term errors) default: 'ft' alg -- Deconvolution algorithm Options: 'clark', 'hogbom', 'multiscale' default: 'clark' cyclefactor -- Controls the threshhold at which the deconvolution cycle will pause to degrid and subtract the model from the visibilities (Cotton-Schwab (CS) major cycle). With poor PSFs, reconcile often (cyclefactor=4 or 5) for reliability. With good PSFs, use cyclefactor = 1.5 to 2.0 for speed. Note: threshold = cyclefactor * max sidelobe * max residual default: 1.5; example: cyclefactor=4 cyclefactor=0 allows the user to control number of CS major cycle >>> majorcycles -- integer number of CS major cycles to do default: 1; example: majorcycles=10 niter -- Maximum number iterations, if niter=0, then no CLEANing is done ("invert" only) default: 500; example: niter=5000 threshold -- Flux level (residual peak) at which to stop CLEANing default: '0.0mJy'; example: threshold='2.3mJy' (always include units) threshold='0.0023Jy' threshold='0.0023Jy/beam' (okay also) weighting -- Weighting to apply to visibilities: Options: 'natural','uniform','briggs', 'superuniform','radial' default: 'natural'; example: weighting='uniform'; scales -- list of scales in pixel for multiscale clean default: [0] example: scales=[0, 3, 10] mode -- type of image to be generated Options: 'continuum', 'cube' default: 'continuum' example: mode='cube'; Use with nchan, start, step to specify output image cube. NOTE: mode='velocity' or 'channel' or 'frequency' are aliased to mode='cube' for backward compatibility and comfort. >>> mode='cube' expandable parameters nchan -- Total number of channels in the output image. Example: nchan=100. Default: -1; Automatically selects enough channels to cover data selected by 'spw' and consistent with 'start' and 'step' It is often easiest to leave nchan at the default value. start -- First channel, velocity, or frequency. if start is an integer pclean will assume it is the a channel index if start is in units of velocity or frequency it will take it as such If the user use the the ms channel as starting pclean will assign the first channel of the image to the data channel frequency in LSRK of the first spw selected at the first time seen in the data and the direction of the source selected. If the data is not in the LSRK frame the user should be aware that the data channel indicated may not fall on the first image channel as time goes. example:start=5 start can be in units of frequency or velocity too When velocity units is used it is obvious then that it is referring to the line whose restfrequency is provided by the user or is default one for the source in the MS/SOURCE table. examples: start='5.0km/s', or start='22.3GHz'. width -- Output channel width should be in the same units as start default=1; >1 indicates channel averaging if start is an integer, width has to be an integer defining the image channel width by the number of channels of first spectral window selected example: width=4. when start is in frequency or velocity units then the width has to be in the same units. default=''; examples: width='1.0km/s', or width='24.2kHz'. interactive -- Create a mask interactively or not. interactive clean allows the user to build the cleaning mask interactively using the viewer. default: False; example: interactive=True The viewer will open with the image displayed. Select the region for the mask and double click in the middle of it. >>> npercycle -- Number of iteration in between viewer interactions. default=100 pbcor -- Output primary beam-corrected image If pbcor=False, the final output image is NOT corrected for the PB pattern (particularly important for mosaics), and therefore is not "flux correct". Correction can also be done after the fact using immath to divide <imagename>.image by the <imagename>.flux image. default: pbcor=False; output un-corrected image example: pbcor=True; output pb-corrected image (masked outside minpb) >>> minpb -- Minimum PB level to use for pb-correction and pb-based masking. default=0.2; example: minpb=0.01 When ftmachine is *not* 'mosaic' : minpb is applied to the flux image (sensitivity-weighted pb). When ftmachine='mosaic' : minpb is applied to the flux.pbcoverage image overwrite -- If False use existing model image of same name to continue clean if True the imagename.model and other associated images are overwitten if they exist default: True timerange -- Select data based on time range: default: '' (all); examples, timerange = 'YYYY/MM/DD/hh:mm:ss~YYYY/MM/DD/hh:mm:ss' Note: if YYYY/MM/DD is missing date defaults to first day in data set timerange='09:14:0~09:54:0' picks 40 min on first day timerange='25:00:00~27:30:00' picks 1 hr to 3 hr 30min on NEXT day timerange='09:44:00' pick data within one integration of time timerange='>10:24:00' data after this time For multiple MS input, a list of timerange strings can be used: uvrange -- Select data within uvrange (default units meters) default: '' (all); example: uvrange='0~1000klambda'; uvrange from 0-1000 kilo-lambda uvrange='>4klambda';uvranges greater than 4 kilo lambda antenna -- Select data based on antenna/baseline default: '' (all) If antenna string is a non-negative integer, it is assumed to be an antenna index, otherwise, it is considered an antenna name. antenna='5&6'; baseline between antenna index 5 and index 6. antenna='VA05&VA06'; baseline between VLA antenna 5 and 6. antenna='5&6;7&8'; baselines 5-6 and 7-8 antenna='5'; all baselines with antenna index 5 antenna='05'; all baselines with antenna number 05 (VLA old name) antenna='5,6,9'; all baselines with antennas 5,6,9 index number scan -- Scan number range. default: '' (all) example: scan='1~5 observation -- Observation ID range. default: '' (all) example: observation='1~5' clusterdef -- Name of a file that contains the cluster definition. NOTE: there is a chapter in the cookbook on how to define this file If clusterdef='' (the default) then all the cores, if possible, of the machine on which casapy is run will be used. Example of a cube imaging run: pclean(vis="ngc5921.ms.contsub",imagename="loulou",imsize=[2500, 2500], cell=['15.0arcsec', '15.0arcsec'],phasecenter="",stokes="I",field="0",spw="*", ftmachine="ft",alg="hogbom",majorcycles=2, niter=6000,gain=0.1, threshold="8mJy",weighting="briggs",robust=0.5,npixels=0,mode="cube", start=5,nchan=46,width=1,interactive=True,overwrite=True,uvtaper=False, outertaper=[''],pbcor=True) Example of a continuum run: pclean(vis='sim100g_4chan15kRows.ms', imagename='hundredG_cont', imsize=[1500, 1500], cell=['0.135arcsec', '0.135arcsec'], mode='continuum', phasecenter='0', field='0', spw='*', ftmachine='wproject', wprojplanes=128, threshold='0.1mJy', majorcycles=4, niter=10000, alg='clark', weighting='natural', overwrite=True)
Definition at line 46 of file pclean_cli.py.
def pclean_cli.pclean_cli_.check_params | ( | self, | |
param = None , |
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value = None , |
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ipython_globals = None |
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) |
Definition at line 640 of file pclean_cli.py.
References clearstat_cli.clearstat_cli_.__globals__, listfits_cli.listfits_cli_.__globals__, clearplot_cli.clearplot_cli_.__globals__, listhistory_cli.listhistory_cli_.__globals__, importfitsidi_cli.importfitsidi_cli_.__globals__, find_cli.find_cli_.__globals__, asdmsummary_cli.asdmsummary_cli_.__globals__, importgmrt_cli.importgmrt_cli_.__globals__, conjugatevis_cli.conjugatevis_cli_.__globals__, importfits_cli.importfits_cli_.__globals__, imreframe_cli.imreframe_cli_.__globals__, importuvfits_cli.importuvfits_cli_.__globals__, msview_cli.msview_cli_.__globals__, flagmanager_cli.flagmanager_cli_.__globals__, delmod_cli.delmod_cli_.__globals__, exportfits_cli.exportfits_cli_.__globals__, caltabconvert_cli.caltabconvert_cli_.__globals__, hanningsmooth_cli.hanningsmooth_cli_.__globals__, boxit_cli.boxit_cli_.__globals__, listsdm_cli.listsdm_cli_.__globals__, calstat_cli.calstat_cli_.__globals__, deconvolve_cli.deconvolve_cli_.__globals__, clearcal_cli.clearcal_cli_.__globals__, fixvis_cli.fixvis_cli_.__globals__, imregrid_cli.imregrid_cli_.__globals__, fixplanets_cli.fixplanets_cli_.__globals__, imsubimage_cli.imsubimage_cli_.__globals__, impbcor_cli.impbcor_cli_.__globals__, exportasdm_cli.exportasdm_cli_.__globals__, imcontsub_cli.imcontsub_cli_.__globals__, ft_cli.ft_cli_.__globals__, browsetable_cli.browsetable_cli_.__globals__, feather_cli.feather_cli_.__globals__, msmoments_cli.msmoments_cli_.__globals__, listpartition_cli.listpartition_cli_.__globals__, importvla_cli.importvla_cli_.__globals__, imtrans_cli.imtrans_cli_.__globals__, imcollapse_cli.imcollapse_cli_.__globals__, listobs_cli.listobs_cli_.__globals__, exportuvfits_cli.exportuvfits_cli_.__globals__, concat_cli.concat_cli_.__globals__, immoments_cli.immoments_cli_.__globals__, imval_cli.imval_cli_.__globals__, fluxscale_cli.fluxscale_cli_.__globals__, imsmooth_cli.imsmooth_cli_.__globals__, csvclean_cli.csvclean_cli_.__globals__, listvis_cli.listvis_cli_.__globals__, imview_cli.imview_cli_.__globals__, importasdm_cli.importasdm_cli_.__globals__, imstat_cli.imstat_cli_.__globals__, accum_cli.accum_cli_.__globals__, imhead_cli.imhead_cli_.__globals__, listcal_cli.listcal_cli_.__globals__, blcal_cli.blcal_cli_.__globals__, makemask_cli.makemask_cli_.__globals__, applycal_cli.applycal_cli_.__globals__, cvel_cli.cvel_cli_.__globals__, importevla_cli.importevla_cli_.__globals__, partition_cli.partition_cli_.__globals__, imfit_cli.imfit_cli_.__globals__, gaincal_cli.gaincal_cli_.__globals__, bandpass_cli.bandpass_cli_.__globals__, immath_cli.immath_cli_.__globals__, mosaic_cli.mosaic_cli_.__globals__, gencal_cli.gencal_cli_.__globals__, pclean_cli.pclean_cli_.__globals__, autoclean_cli.autoclean_cli_.__globals__, flagcmd_cli.flagcmd_cli_.__globals__, clean_cli.clean_cli_.__globals__, and flagdata_cli.flagdata_cli_.__globals__.
def pclean_cli.pclean_cli_.defaults | ( | self, | |
param = None , |
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ipython_globals = None , |
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paramvalue = None , |
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subparam = None |
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) |
Definition at line 533 of file pclean_cli.py.
References clearstat_cli.clearstat_cli_.__globals__, listfits_cli.listfits_cli_.__globals__, clearplot_cli.clearplot_cli_.__globals__, listhistory_cli.listhistory_cli_.__globals__, importfitsidi_cli.importfitsidi_cli_.__globals__, find_cli.find_cli_.__globals__, asdmsummary_cli.asdmsummary_cli_.__globals__, importgmrt_cli.importgmrt_cli_.__globals__, conjugatevis_cli.conjugatevis_cli_.__globals__, importfits_cli.importfits_cli_.__globals__, imreframe_cli.imreframe_cli_.__globals__, importuvfits_cli.importuvfits_cli_.__globals__, msview_cli.msview_cli_.__globals__, flagmanager_cli.flagmanager_cli_.__globals__, delmod_cli.delmod_cli_.__globals__, exportfits_cli.exportfits_cli_.__globals__, caltabconvert_cli.caltabconvert_cli_.__globals__, hanningsmooth_cli.hanningsmooth_cli_.__globals__, boxit_cli.boxit_cli_.__globals__, listsdm_cli.listsdm_cli_.__globals__, calstat_cli.calstat_cli_.__globals__, deconvolve_cli.deconvolve_cli_.__globals__, clearcal_cli.clearcal_cli_.__globals__, fixvis_cli.fixvis_cli_.__globals__, imregrid_cli.imregrid_cli_.__globals__, fixplanets_cli.fixplanets_cli_.__globals__, imsubimage_cli.imsubimage_cli_.__globals__, impbcor_cli.impbcor_cli_.__globals__, exportasdm_cli.exportasdm_cli_.__globals__, imcontsub_cli.imcontsub_cli_.__globals__, ft_cli.ft_cli_.__globals__, browsetable_cli.browsetable_cli_.__globals__, feather_cli.feather_cli_.__globals__, msmoments_cli.msmoments_cli_.__globals__, listpartition_cli.listpartition_cli_.__globals__, importvla_cli.importvla_cli_.__globals__, imtrans_cli.imtrans_cli_.__globals__, imcollapse_cli.imcollapse_cli_.__globals__, listobs_cli.listobs_cli_.__globals__, exportuvfits_cli.exportuvfits_cli_.__globals__, concat_cli.concat_cli_.__globals__, immoments_cli.immoments_cli_.__globals__, imval_cli.imval_cli_.__globals__, fluxscale_cli.fluxscale_cli_.__globals__, imsmooth_cli.imsmooth_cli_.__globals__, csvclean_cli.csvclean_cli_.__globals__, listvis_cli.listvis_cli_.__globals__, imview_cli.imview_cli_.__globals__, importasdm_cli.importasdm_cli_.__globals__, imstat_cli.imstat_cli_.__globals__, accum_cli.accum_cli_.__globals__, imhead_cli.imhead_cli_.__globals__, listcal_cli.listcal_cli_.__globals__, blcal_cli.blcal_cli_.__globals__, makemask_cli.makemask_cli_.__globals__, applycal_cli.applycal_cli_.__globals__, cvel_cli.cvel_cli_.__globals__, importevla_cli.importevla_cli_.__globals__, partition_cli.partition_cli_.__globals__, imfit_cli.imfit_cli_.__globals__, gaincal_cli.gaincal_cli_.__globals__, bandpass_cli.bandpass_cli_.__globals__, immath_cli.immath_cli_.__globals__, mosaic_cli.mosaic_cli_.__globals__, gencal_cli.gencal_cli_.__globals__, pclean_cli.pclean_cli_.__globals__, autoclean_cli.autoclean_cli_.__globals__, flagcmd_cli.flagcmd_cli_.__globals__, clean_cli.clean_cli_.__globals__, flagdata_cli.flagdata_cli_.__globals__, clearstat_cli.clearstat_cli_.itsdefault(), listfits_cli.listfits_cli_.itsdefault(), clearplot_cli.clearplot_cli_.itsdefault(), listhistory_cli.listhistory_cli_.itsdefault(), find_cli.find_cli_.itsdefault(), asdmsummary_cli.asdmsummary_cli_.itsdefault(), importfitsidi_cli.importfitsidi_cli_.itsdefault(), importgmrt_cli.importgmrt_cli_.itsdefault(), importuvfits_cli.importuvfits_cli_.itsdefault(), conjugatevis_cli.conjugatevis_cli_.itsdefault(), listsdm_cli.listsdm_cli_.itsdefault(), importfits_cli.importfits_cli_.itsdefault(), hanningsmooth_cli.hanningsmooth_cli_.itsdefault(), caltabconvert_cli.caltabconvert_cli_.itsdefault(), imreframe_cli.imreframe_cli_.itsdefault(), delmod_cli.delmod_cli_.itsdefault(), flagmanager_cli.flagmanager_cli_.itsdefault(), clearcal_cli.clearcal_cli_.itsdefault(), calstat_cli.calstat_cli_.itsdefault(), listpartition_cli.listpartition_cli_.itsdefault(), fixplanets_cli.fixplanets_cli_.itsdefault(), exportfits_cli.exportfits_cli_.itsdefault(), fixvis_cli.fixvis_cli_.itsdefault(), msview_cli.msview_cli_.itsdefault(), boxit_cli.boxit_cli_.itsdefault(), imregrid_cli.imregrid_cli_.itsdefault(), imtrans_cli.imtrans_cli_.itsdefault(), feather_cli.feather_cli_.itsdefault(), browsetable_cli.browsetable_cli_.itsdefault(), imsubimage_cli.imsubimage_cli_.itsdefault(), imcontsub_cli.imcontsub_cli_.itsdefault(), msmoments_cli.msmoments_cli_.itsdefault(), ft_cli.ft_cli_.itsdefault(), exportasdm_cli.exportasdm_cli_.itsdefault(), deconvolve_cli.deconvolve_cli_.itsdefault(), impbcor_cli.impbcor_cli_.itsdefault(), importvla_cli.importvla_cli_.itsdefault(), imcollapse_cli.imcollapse_cli_.itsdefault(), imval_cli.imval_cli_.itsdefault(), concat_cli.concat_cli_.itsdefault(), listobs_cli.listobs_cli_.itsdefault(), fluxscale_cli.fluxscale_cli_.itsdefault(), imview_cli.imview_cli_.itsdefault(), exportuvfits_cli.exportuvfits_cli_.itsdefault(), immoments_cli.immoments_cli_.itsdefault(), imsmooth_cli.imsmooth_cli_.itsdefault(), listcal_cli.listcal_cli_.itsdefault(), accum_cli.accum_cli_.itsdefault(), csvclean_cli.csvclean_cli_.itsdefault(), imhead_cli.imhead_cli_.itsdefault(), imstat_cli.imstat_cli_.itsdefault(), listvis_cli.listvis_cli_.itsdefault(), makemask_cli.makemask_cli_.itsdefault(), importasdm_cli.importasdm_cli_.itsdefault(), blcal_cli.blcal_cli_.itsdefault(), applycal_cli.applycal_cli_.itsdefault(), importevla_cli.importevla_cli_.itsdefault(), gencal_cli.gencal_cli_.itsdefault(), cvel_cli.cvel_cli_.itsdefault(), partition_cli.partition_cli_.itsdefault(), imfit_cli.imfit_cli_.itsdefault(), immath_cli.immath_cli_.itsdefault(), bandpass_cli.bandpass_cli_.itsdefault(), gaincal_cli.gaincal_cli_.itsdefault(), mosaic_cli.mosaic_cli_.itsdefault(), pclean_cli.pclean_cli_.itsdefault(), autoclean_cli.autoclean_cli_.itsdefault(), flagcmd_cli.flagcmd_cli_.itsdefault(), clean_cli.clean_cli_.itsdefault(), and flagdata_cli.flagdata_cli_.itsdefault().
def pclean_cli.pclean_cli_.description | ( | self, | |
key = 'pclean' , |
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subkey = None |
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) |
Definition at line 671 of file pclean_cli.py.
def pclean_cli.pclean_cli_.itsdefault | ( | self, | |
paramname | |||
) |
Definition at line 725 of file pclean_cli.py.
References accum_cli.accum_cli_.parameters, pclean_cli.pclean_cli_.parameters, partition_cli.partition_cli_.parameters, msview_cli.msview_cli_.parameters, msmoments_cli.msmoments_cli_.parameters, mosaic_cli.mosaic_cli_.parameters, makemask_cli.makemask_cli_.parameters, listvis_cli.listvis_cli_.parameters, listsdm_cli.listsdm_cli_.parameters, listpartition_cli.listpartition_cli_.parameters, listobs_cli.listobs_cli_.parameters, listhistory_cli.listhistory_cli_.parameters, listfits_cli.listfits_cli_.parameters, listcal_cli.listcal_cli_.parameters, imview_cli.imview_cli_.parameters, imval_cli.imval_cli_.parameters, imtrans_cli.imtrans_cli_.parameters, imsubimage_cli.imsubimage_cli_.parameters, imstat_cli.imstat_cli_.parameters, imsmooth_cli.imsmooth_cli_.parameters, imregrid_cli.imregrid_cli_.parameters, imreframe_cli.imreframe_cli_.parameters, importvla_cli.importvla_cli_.parameters, importuvfits_cli.importuvfits_cli_.parameters, importgmrt_cli.importgmrt_cli_.parameters, importfitsidi_cli.importfitsidi_cli_.parameters, importfits_cli.importfits_cli_.parameters, importevla_cli.importevla_cli_.parameters, importasdm_cli.importasdm_cli_.parameters, impbcor_cli.impbcor_cli_.parameters, immoments_cli.immoments_cli_.parameters, immath_cli.immath_cli_.parameters, imhead_cli.imhead_cli_.parameters, imfit_cli.imfit_cli_.parameters, imcontsub_cli.imcontsub_cli_.parameters, imcollapse_cli.imcollapse_cli_.parameters, hanningsmooth_cli.hanningsmooth_cli_.parameters, gencal_cli.gencal_cli_.parameters, gaincal_cli.gaincal_cli_.parameters, ft_cli.ft_cli_.parameters, fluxscale_cli.fluxscale_cli_.parameters, flagmanager_cli.flagmanager_cli_.parameters, flagdata_cli.flagdata_cli_.parameters, flagcmd_cli.flagcmd_cli_.parameters, fixvis_cli.fixvis_cli_.parameters, fixplanets_cli.fixplanets_cli_.parameters, find_cli.find_cli_.parameters, feather_cli.feather_cli_.parameters, exportuvfits_cli.exportuvfits_cli_.parameters, exportfits_cli.exportfits_cli_.parameters, exportasdm_cli.exportasdm_cli_.parameters, delmod_cli.delmod_cli_.parameters, deconvolve_cli.deconvolve_cli_.parameters, cvel_cli.cvel_cli_.parameters, csvclean_cli.csvclean_cli_.parameters, conjugatevis_cli.conjugatevis_cli_.parameters, concat_cli.concat_cli_.parameters, clearstat_cli.clearstat_cli_.parameters, clearplot_cli.clearplot_cli_.parameters, clearcal_cli.clearcal_cli_.parameters, clean_cli.clean_cli_.parameters, caltabconvert_cli.caltabconvert_cli_.parameters, calstat_cli.calstat_cli_.parameters, browsetable_cli.browsetable_cli_.parameters, boxit_cli.boxit_cli_.parameters, blcal_cli.blcal_cli_.parameters, bandpass_cli.bandpass_cli_.parameters, autoclean_cli.autoclean_cli_.parameters, asdmsummary_cli.asdmsummary_cli_.parameters, and applycal_cli.applycal_cli_.parameters.
Referenced by rmtables_cli.rmtables_cli_.defaults(), uvsub_cli.uvsub_cli_.defaults(), uvcontsub2_cli.uvcontsub2_cli_.defaults(), plotweather_cli.plotweather_cli_.defaults(), plotants_cli.plotants_cli_.defaults(), smoothcal_cli.smoothcal_cli_.defaults(), tclean_cli.tclean_cli_.defaults(), splattotable_cli.splattotable_cli_.defaults(), sdflagmanager_cli.sdflagmanager_cli_.defaults(), testconcat_cli.testconcat_cli_.defaults(), sdlist_cli.sdlist_cli_.defaults(), viewer_cli.viewer_cli_.defaults(), sdscale_cli.sdscale_cli_.defaults(), slsearch_cli.slsearch_cli_.defaults(), peel_cli.peel_cli_.defaults(), predictcomp_cli.predictcomp_cli_.defaults(), uvcontsub_cli.uvcontsub_cli_.defaults(), wvrgcal_cli.wvrgcal_cli_.defaults(), ssoflux_cli.ssoflux_cli_.defaults(), vishead_cli.vishead_cli_.defaults(), uvcontsub3_cli.uvcontsub3_cli_.defaults(), sdimprocess_cli.sdimprocess_cli_.defaults(), virtualconcat_cli.virtualconcat_cli_.defaults(), sdsmooth_cli.sdsmooth_cli_.defaults(), visstat_cli.visstat_cli_.defaults(), widebandpbcor_cli.widebandpbcor_cli_.defaults(), sdcoadd_cli.sdcoadd_cli_.defaults(), uvmodelfit_cli.uvmodelfit_cli_.defaults(), sdsave_cli.sdsave_cli_.defaults(), simanalyze_cli.simanalyze_cli_.defaults(), sdmath_cli.sdmath_cli_.defaults(), sdgrid_cli.sdgrid_cli_.defaults(), sdtpimaging_cli.sdtpimaging_cli_.defaults(), sdstat_cli.sdstat_cli_.defaults(), split_cli.split_cli_.defaults(), sdimaging_cli.sdimaging_cli_.defaults(), statwt_cli.statwt_cli_.defaults(), sdflag_cli.sdflag_cli_.defaults(), simalma_cli.simalma_cli_.defaults(), sdfit_cli.sdfit_cli_.defaults(), sdcal_cli.sdcal_cli_.defaults(), simobserve_cli.simobserve_cli_.defaults(), polcal_cli.polcal_cli_.defaults(), sdbaseline_cli.sdbaseline_cli_.defaults(), setjy_cli.setjy_cli_.defaults(), widefield_cli.widefield_cli_.defaults(), pclean_cli.pclean_cli_.defaults(), plotxy_cli.plotxy_cli_.defaults(), specfit_cli.specfit_cli_.defaults(), plotms_cli.plotms_cli_.defaults(), and sdreduce_cli.sdreduce_cli_.defaults().
def pclean_cli.pclean_cli_.paramgui | ( | self, | |
useGlobals = True , |
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ipython_globals = None |
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) |
Opens a parameter GUI for this task. If useGlobals is true, then any relevant global parameter settings are used.
Definition at line 509 of file pclean_cli.py.
References clearstat_cli.clearstat_cli_.__globals__, listfits_cli.listfits_cli_.__globals__, clearplot_cli.clearplot_cli_.__globals__, listhistory_cli.listhistory_cli_.__globals__, importfitsidi_cli.importfitsidi_cli_.__globals__, find_cli.find_cli_.__globals__, asdmsummary_cli.asdmsummary_cli_.__globals__, importgmrt_cli.importgmrt_cli_.__globals__, conjugatevis_cli.conjugatevis_cli_.__globals__, importfits_cli.importfits_cli_.__globals__, imreframe_cli.imreframe_cli_.__globals__, importuvfits_cli.importuvfits_cli_.__globals__, msview_cli.msview_cli_.__globals__, flagmanager_cli.flagmanager_cli_.__globals__, delmod_cli.delmod_cli_.__globals__, exportfits_cli.exportfits_cli_.__globals__, caltabconvert_cli.caltabconvert_cli_.__globals__, hanningsmooth_cli.hanningsmooth_cli_.__globals__, boxit_cli.boxit_cli_.__globals__, listsdm_cli.listsdm_cli_.__globals__, calstat_cli.calstat_cli_.__globals__, deconvolve_cli.deconvolve_cli_.__globals__, clearcal_cli.clearcal_cli_.__globals__, fixvis_cli.fixvis_cli_.__globals__, imregrid_cli.imregrid_cli_.__globals__, fixplanets_cli.fixplanets_cli_.__globals__, imsubimage_cli.imsubimage_cli_.__globals__, impbcor_cli.impbcor_cli_.__globals__, exportasdm_cli.exportasdm_cli_.__globals__, imcontsub_cli.imcontsub_cli_.__globals__, ft_cli.ft_cli_.__globals__, browsetable_cli.browsetable_cli_.__globals__, feather_cli.feather_cli_.__globals__, msmoments_cli.msmoments_cli_.__globals__, listpartition_cli.listpartition_cli_.__globals__, importvla_cli.importvla_cli_.__globals__, imtrans_cli.imtrans_cli_.__globals__, imcollapse_cli.imcollapse_cli_.__globals__, listobs_cli.listobs_cli_.__globals__, exportuvfits_cli.exportuvfits_cli_.__globals__, concat_cli.concat_cli_.__globals__, immoments_cli.immoments_cli_.__globals__, imval_cli.imval_cli_.__globals__, fluxscale_cli.fluxscale_cli_.__globals__, imsmooth_cli.imsmooth_cli_.__globals__, csvclean_cli.csvclean_cli_.__globals__, listvis_cli.listvis_cli_.__globals__, imview_cli.imview_cli_.__globals__, importasdm_cli.importasdm_cli_.__globals__, imstat_cli.imstat_cli_.__globals__, accum_cli.accum_cli_.__globals__, imhead_cli.imhead_cli_.__globals__, listcal_cli.listcal_cli_.__globals__, blcal_cli.blcal_cli_.__globals__, makemask_cli.makemask_cli_.__globals__, applycal_cli.applycal_cli_.__globals__, cvel_cli.cvel_cli_.__globals__, importevla_cli.importevla_cli_.__globals__, partition_cli.partition_cli_.__globals__, imfit_cli.imfit_cli_.__globals__, gaincal_cli.gaincal_cli_.__globals__, bandpass_cli.bandpass_cli_.__globals__, immath_cli.immath_cli_.__globals__, mosaic_cli.mosaic_cli_.__globals__, gencal_cli.gencal_cli_.__globals__, pclean_cli.pclean_cli_.__globals__, autoclean_cli.autoclean_cli_.__globals__, flagcmd_cli.flagcmd_cli_.__globals__, clean_cli.clean_cli_.__globals__, and flagdata_cli.flagdata_cli_.__globals__.
def pclean_cli.pclean_cli_.result | ( | self, | |
key = None |
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) |
Definition at line 33 of file pclean_cli.py.
References accum_cli.accum_cli_.__async__, pclean_cli.pclean_cli_.__async__, partition_cli.partition_cli_.__async__, msview_cli.msview_cli_.__async__, msmoments_cli.msmoments_cli_.__async__, mosaic_cli.mosaic_cli_.__async__, makemask_cli.makemask_cli_.__async__, listvis_cli.listvis_cli_.__async__, listsdm_cli.listsdm_cli_.__async__, listpartition_cli.listpartition_cli_.__async__, listobs_cli.listobs_cli_.__async__, listhistory_cli.listhistory_cli_.__async__, listfits_cli.listfits_cli_.__async__, listcal_cli.listcal_cli_.__async__, imview_cli.imview_cli_.__async__, imval_cli.imval_cli_.__async__, imtrans_cli.imtrans_cli_.__async__, imsubimage_cli.imsubimage_cli_.__async__, imstat_cli.imstat_cli_.__async__, imsmooth_cli.imsmooth_cli_.__async__, imregrid_cli.imregrid_cli_.__async__, imreframe_cli.imreframe_cli_.__async__, importvla_cli.importvla_cli_.__async__, importuvfits_cli.importuvfits_cli_.__async__, importgmrt_cli.importgmrt_cli_.__async__, importfitsidi_cli.importfitsidi_cli_.__async__, importfits_cli.importfits_cli_.__async__, importevla_cli.importevla_cli_.__async__, importasdm_cli.importasdm_cli_.__async__, impbcor_cli.impbcor_cli_.__async__, immoments_cli.immoments_cli_.__async__, immath_cli.immath_cli_.__async__, imhead_cli.imhead_cli_.__async__, imfit_cli.imfit_cli_.__async__, imcontsub_cli.imcontsub_cli_.__async__, imcollapse_cli.imcollapse_cli_.__async__, hanningsmooth_cli.hanningsmooth_cli_.__async__, gencal_cli.gencal_cli_.__async__, gaincal_cli.gaincal_cli_.__async__, ft_cli.ft_cli_.__async__, fluxscale_cli.fluxscale_cli_.__async__, flagmanager_cli.flagmanager_cli_.__async__, flagdata_cli.flagdata_cli_.__async__, flagcmd_cli.flagcmd_cli_.__async__, fixvis_cli.fixvis_cli_.__async__, fixplanets_cli.fixplanets_cli_.__async__, find_cli.find_cli_.__async__, feather_cli.feather_cli_.__async__, exportuvfits_cli.exportuvfits_cli_.__async__, exportfits_cli.exportfits_cli_.__async__, exportasdm_cli.exportasdm_cli_.__async__, delmod_cli.delmod_cli_.__async__, deconvolve_cli.deconvolve_cli_.__async__, cvel_cli.cvel_cli_.__async__, csvclean_cli.csvclean_cli_.__async__, conjugatevis_cli.conjugatevis_cli_.__async__, concat_cli.concat_cli_.__async__, clearstat_cli.clearstat_cli_.__async__, clearplot_cli.clearplot_cli_.__async__, clearcal_cli.clearcal_cli_.__async__, clean_cli.clean_cli_.__async__, caltabconvert_cli.caltabconvert_cli_.__async__, calstat_cli.calstat_cli_.__async__, browsetable_cli.browsetable_cli_.__async__, boxit_cli.boxit_cli_.__async__, blcal_cli.blcal_cli_.__async__, bandpass_cli.bandpass_cli_.__async__, autoclean_cli.autoclean_cli_.__async__, asdmsummary_cli.asdmsummary_cli_.__async__, and applycal_cli.applycal_cli_.__async__.
dictionary pclean_cli.pclean_cli_.__async__ [static, private] |
Definition at line 20 of file pclean_cli.py.
Referenced by pclean_cli.pclean_cli_.result(), wvrgcal_cli.wvrgcal_cli_.result(), widefield_cli.widefield_cli_.result(), widebandpbcor_cli.widebandpbcor_cli_.result(), visstat_cli.visstat_cli_.result(), vishead_cli.vishead_cli_.result(), virtualconcat_cli.virtualconcat_cli_.result(), viewer_cli.viewer_cli_.result(), uvsub_cli.uvsub_cli_.result(), uvmodelfit_cli.uvmodelfit_cli_.result(), uvcontsub_cli.uvcontsub_cli_.result(), uvcontsub3_cli.uvcontsub3_cli_.result(), uvcontsub2_cli.uvcontsub2_cli_.result(), testconcat_cli.testconcat_cli_.result(), tclean_cli.tclean_cli_.result(), statwt_cli.statwt_cli_.result(), ssoflux_cli.ssoflux_cli_.result(), split_cli.split_cli_.result(), splattotable_cli.splattotable_cli_.result(), specfit_cli.specfit_cli_.result(), smoothcal_cli.smoothcal_cli_.result(), slsearch_cli.slsearch_cli_.result(), simobserve_cli.simobserve_cli_.result(), simanalyze_cli.simanalyze_cli_.result(), simalma_cli.simalma_cli_.result(), setjy_cli.setjy_cli_.result(), sdtpimaging_cli.sdtpimaging_cli_.result(), sdstat_cli.sdstat_cli_.result(), sdsmooth_cli.sdsmooth_cli_.result(), sdscale_cli.sdscale_cli_.result(), sdsave_cli.sdsave_cli_.result(), sdreduce_cli.sdreduce_cli_.result(), sdplot_cli.sdplot_cli_.result(), sdmath_cli.sdmath_cli_.result(), sdlist_cli.sdlist_cli_.result(), sdimprocess_cli.sdimprocess_cli_.result(), sdimaging_cli.sdimaging_cli_.result(), sdgrid_cli.sdgrid_cli_.result(), sdflagmanager_cli.sdflagmanager_cli_.result(), sdflag_cli.sdflag_cli_.result(), sdfit_cli.sdfit_cli_.result(), sdcoadd_cli.sdcoadd_cli_.result(), sdcal_cli.sdcal_cli_.result(), sdbaseline_cli.sdbaseline_cli_.result(), rmtables_cli.rmtables_cli_.result(), predictcomp_cli.predictcomp_cli_.result(), polcal_cli.polcal_cli_.result(), plotxy_cli.plotxy_cli_.result(), plotweather_cli.plotweather_cli_.result(), plotuv_cli.plotuv_cli_.result(), plotms_cli.plotms_cli_.result(), plotcal_cli.plotcal_cli_.result(), plotants_cli.plotants_cli_.result(), and peel_cli.peel_cli_.result().
pclean_cli.pclean_cli_.__bases__ [private] |
Definition at line 27 of file pclean_cli.py.
pclean_cli.pclean_cli_.__doc__ [private] |
Definition at line 28 of file pclean_cli.py.
pclean_cli.pclean_cli_.__globals__ [private] |
Definition at line 313 of file pclean_cli.py.
Referenced by rmtables_cli.rmtables_cli_.check_params(), uvsub_cli.uvsub_cli_.check_params(), plotweather_cli.plotweather_cli_.check_params(), uvcontsub2_cli.uvcontsub2_cli_.check_params(), plotants_cli.plotants_cli_.check_params(), smoothcal_cli.smoothcal_cli_.check_params(), splattotable_cli.splattotable_cli_.check_params(), sdflagmanager_cli.sdflagmanager_cli_.check_params(), tclean_cli.tclean_cli_.check_params(), testconcat_cli.testconcat_cli_.check_params(), sdlist_cli.sdlist_cli_.check_params(), viewer_cli.viewer_cli_.check_params(), sdscale_cli.sdscale_cli_.check_params(), peel_cli.peel_cli_.check_params(), uvcontsub_cli.uvcontsub_cli_.check_params(), slsearch_cli.slsearch_cli_.check_params(), ssoflux_cli.ssoflux_cli_.check_params(), predictcomp_cli.predictcomp_cli_.check_params(), vishead_cli.vishead_cli_.check_params(), wvrgcal_cli.wvrgcal_cli_.check_params(), uvcontsub3_cli.uvcontsub3_cli_.check_params(), sdimprocess_cli.sdimprocess_cli_.check_params(), virtualconcat_cli.virtualconcat_cli_.check_params(), sdsmooth_cli.sdsmooth_cli_.check_params(), visstat_cli.visstat_cli_.check_params(), widebandpbcor_cli.widebandpbcor_cli_.check_params(), uvmodelfit_cli.uvmodelfit_cli_.check_params(), sdcoadd_cli.sdcoadd_cli_.check_params(), simanalyze_cli.simanalyze_cli_.check_params(), sdsave_cli.sdsave_cli_.check_params(), sdmath_cli.sdmath_cli_.check_params(), sdgrid_cli.sdgrid_cli_.check_params(), sdtpimaging_cli.sdtpimaging_cli_.check_params(), split_cli.split_cli_.check_params(), sdstat_cli.sdstat_cli_.check_params(), statwt_cli.statwt_cli_.check_params(), sdimaging_cli.sdimaging_cli_.check_params(), sdflag_cli.sdflag_cli_.check_params(), simalma_cli.simalma_cli_.check_params(), sdfit_cli.sdfit_cli_.check_params(), simobserve_cli.simobserve_cli_.check_params(), polcal_cli.polcal_cli_.check_params(), sdcal_cli.sdcal_cli_.check_params(), setjy_cli.setjy_cli_.check_params(), sdbaseline_cli.sdbaseline_cli_.check_params(), widefield_cli.widefield_cli_.check_params(), pclean_cli.pclean_cli_.check_params(), plotxy_cli.plotxy_cli_.check_params(), specfit_cli.specfit_cli_.check_params(), sdreduce_cli.sdreduce_cli_.check_params(), plotms_cli.plotms_cli_.check_params(), rmtables_cli.rmtables_cli_.defaults(), uvsub_cli.uvsub_cli_.defaults(), uvcontsub2_cli.uvcontsub2_cli_.defaults(), plotweather_cli.plotweather_cli_.defaults(), plotants_cli.plotants_cli_.defaults(), smoothcal_cli.smoothcal_cli_.defaults(), tclean_cli.tclean_cli_.defaults(), splattotable_cli.splattotable_cli_.defaults(), sdflagmanager_cli.sdflagmanager_cli_.defaults(), testconcat_cli.testconcat_cli_.defaults(), sdlist_cli.sdlist_cli_.defaults(), viewer_cli.viewer_cli_.defaults(), sdscale_cli.sdscale_cli_.defaults(), slsearch_cli.slsearch_cli_.defaults(), peel_cli.peel_cli_.defaults(), predictcomp_cli.predictcomp_cli_.defaults(), wvrgcal_cli.wvrgcal_cli_.defaults(), uvcontsub_cli.uvcontsub_cli_.defaults(), ssoflux_cli.ssoflux_cli_.defaults(), vishead_cli.vishead_cli_.defaults(), uvcontsub3_cli.uvcontsub3_cli_.defaults(), sdimprocess_cli.sdimprocess_cli_.defaults(), virtualconcat_cli.virtualconcat_cli_.defaults(), sdsmooth_cli.sdsmooth_cli_.defaults(), visstat_cli.visstat_cli_.defaults(), widebandpbcor_cli.widebandpbcor_cli_.defaults(), sdcoadd_cli.sdcoadd_cli_.defaults(), uvmodelfit_cli.uvmodelfit_cli_.defaults(), sdsave_cli.sdsave_cli_.defaults(), simanalyze_cli.simanalyze_cli_.defaults(), sdmath_cli.sdmath_cli_.defaults(), sdgrid_cli.sdgrid_cli_.defaults(), sdtpimaging_cli.sdtpimaging_cli_.defaults(), sdstat_cli.sdstat_cli_.defaults(), split_cli.split_cli_.defaults(), sdimaging_cli.sdimaging_cli_.defaults(), statwt_cli.statwt_cli_.defaults(), sdflag_cli.sdflag_cli_.defaults(), simalma_cli.simalma_cli_.defaults(), sdfit_cli.sdfit_cli_.defaults(), sdcal_cli.sdcal_cli_.defaults(), simobserve_cli.simobserve_cli_.defaults(), polcal_cli.polcal_cli_.defaults(), sdbaseline_cli.sdbaseline_cli_.defaults(), setjy_cli.setjy_cli_.defaults(), widefield_cli.widefield_cli_.defaults(), pclean_cli.pclean_cli_.defaults(), specfit_cli.specfit_cli_.defaults(), sdreduce_cli.sdreduce_cli_.defaults(), rmtables_cli.rmtables_cli_.paramgui(), uvsub_cli.uvsub_cli_.paramgui(), uvcontsub2_cli.uvcontsub2_cli_.paramgui(), plotweather_cli.plotweather_cli_.paramgui(), plotants_cli.plotants_cli_.paramgui(), smoothcal_cli.smoothcal_cli_.paramgui(), tclean_cli.tclean_cli_.paramgui(), splattotable_cli.splattotable_cli_.paramgui(), sdflagmanager_cli.sdflagmanager_cli_.paramgui(), testconcat_cli.testconcat_cli_.paramgui(), sdlist_cli.sdlist_cli_.paramgui(), viewer_cli.viewer_cli_.paramgui(), sdscale_cli.sdscale_cli_.paramgui(), slsearch_cli.slsearch_cli_.paramgui(), peel_cli.peel_cli_.paramgui(), predictcomp_cli.predictcomp_cli_.paramgui(), wvrgcal_cli.wvrgcal_cli_.paramgui(), uvcontsub_cli.uvcontsub_cli_.paramgui(), ssoflux_cli.ssoflux_cli_.paramgui(), vishead_cli.vishead_cli_.paramgui(), uvcontsub3_cli.uvcontsub3_cli_.paramgui(), sdimprocess_cli.sdimprocess_cli_.paramgui(), virtualconcat_cli.virtualconcat_cli_.paramgui(), sdsmooth_cli.sdsmooth_cli_.paramgui(), visstat_cli.visstat_cli_.paramgui(), widebandpbcor_cli.widebandpbcor_cli_.paramgui(), sdcoadd_cli.sdcoadd_cli_.paramgui(), uvmodelfit_cli.uvmodelfit_cli_.paramgui(), sdsave_cli.sdsave_cli_.paramgui(), simanalyze_cli.simanalyze_cli_.paramgui(), sdmath_cli.sdmath_cli_.paramgui(), sdgrid_cli.sdgrid_cli_.paramgui(), sdtpimaging_cli.sdtpimaging_cli_.paramgui(), sdstat_cli.sdstat_cli_.paramgui(), split_cli.split_cli_.paramgui(), sdimaging_cli.sdimaging_cli_.paramgui(), statwt_cli.statwt_cli_.paramgui(), sdflag_cli.sdflag_cli_.paramgui(), simalma_cli.simalma_cli_.paramgui(), sdfit_cli.sdfit_cli_.paramgui(), sdcal_cli.sdcal_cli_.paramgui(), simobserve_cli.simobserve_cli_.paramgui(), polcal_cli.polcal_cli_.paramgui(), sdbaseline_cli.sdbaseline_cli_.paramgui(), setjy_cli.setjy_cli_.paramgui(), widefield_cli.widefield_cli_.paramgui(), pclean_cli.pclean_cli_.paramgui(), specfit_cli.specfit_cli_.paramgui(), and sdreduce_cli.sdreduce_cli_.paramgui().
string pclean_cli.pclean_cli_.__name__ [static, private] |
Definition at line 19 of file pclean_cli.py.
Definition at line 22 of file pclean_cli.py.
Definition at line 30 of file pclean_cli.py.
Referenced by sdflagmanager_cli.sdflagmanager_cli_.itsdefault(), tclean_cli.tclean_cli_.itsdefault(), vishead_cli.vishead_cli_.itsdefault(), predictcomp_cli.predictcomp_cli_.itsdefault(), slsearch_cli.slsearch_cli_.itsdefault(), sdimprocess_cli.sdimprocess_cli_.itsdefault(), wvrgcal_cli.wvrgcal_cli_.itsdefault(), sdsmooth_cli.sdsmooth_cli_.itsdefault(), widebandpbcor_cli.widebandpbcor_cli_.itsdefault(), visstat_cli.visstat_cli_.itsdefault(), uvmodelfit_cli.uvmodelfit_cli_.itsdefault(), sdcoadd_cli.sdcoadd_cli_.itsdefault(), sdsave_cli.sdsave_cli_.itsdefault(), simanalyze_cli.simanalyze_cli_.itsdefault(), sdmath_cli.sdmath_cli_.itsdefault(), sdgrid_cli.sdgrid_cli_.itsdefault(), sdtpimaging_cli.sdtpimaging_cli_.itsdefault(), split_cli.split_cli_.itsdefault(), sdstat_cli.sdstat_cli_.itsdefault(), statwt_cli.statwt_cli_.itsdefault(), sdimaging_cli.sdimaging_cli_.itsdefault(), sdflag_cli.sdflag_cli_.itsdefault(), simalma_cli.simalma_cli_.itsdefault(), sdfit_cli.sdfit_cli_.itsdefault(), polcal_cli.polcal_cli_.itsdefault(), sdcal_cli.sdcal_cli_.itsdefault(), simobserve_cli.simobserve_cli_.itsdefault(), setjy_cli.setjy_cli_.itsdefault(), sdbaseline_cli.sdbaseline_cli_.itsdefault(), pclean_cli.pclean_cli_.itsdefault(), widefield_cli.widefield_cli_.itsdefault(), plotxy_cli.plotxy_cli_.itsdefault(), specfit_cli.specfit_cli_.itsdefault(), sdreduce_cli.sdreduce_cli_.itsdefault(), and plotms_cli.plotms_cli_.itsdefault().
tuple pclean_cli.pclean_cli_.retval [static] |
This function sets the default values but also will return the list of parameters or the default value of a given parameter.
Definition at line 619 of file pclean_cli.py.
tuple pclean_cli.pclean_cli_.retval [static] |
Definition at line 632 of file pclean_cli.py.
pclean_cli.pclean_cli_.rkey [static] |
Handle globals or user over-ride of arguments.
Definition at line 21 of file pclean_cli.py.
string pclean_cli.pclean_cli_.valornotval [static] |
Definition at line 622 of file pclean_cli.py.