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__

Detailed Description

Definition at line 18 of file ssoflux_cli.py.

Constructor & Destructor Documentation

def ssoflux_cli.ssoflux_cli_.__init__ ( self )

Definition at line 26 of file ssoflux_cli.py.

Member Function Documentation

def ssoflux_cli.ssoflux_cli_.__call__	(	self,
		vis = `None`,
		field = `None`,
		spw = `None`,
		modimage = `None`,
		fluxdensity = `None`,
		standard = `None`,
		async = `None`
	)

Fills the model column with the visibilities of a calibrator
       *This is an experimental clone of setjy while flux calibration with
Solar System objects is being tested.  It will eventually be merged
back into setjy.*

       This task sets the model visibility amp and phase of a
       specified source (generally a calibrator).  The simplest way is
       to enter the flux density (I,Q,U,V) explicitly, but this is
       valid only for a point source.

       For an extended source, the clean model (image.model) can be
       specified and the model visibilities associated with this clean
       model is placed in the visibility model column.

       Models are available for 3C48, 3C138, 3C286 between
       1.4 and 43 GHz.  3C147 is available above 13 GHz.  These models
       are scaled to the precise frequency of the data.  Only I source 
       model can be inserted at a time.

       The location of the models are system dependent:  At the AOC and CV,
       the models are in the directory::/usr/lib/casapy/data/nrao/VLA/CalModels
       or /usr/lib64/casapy/data/nrao/VLA/CalModel.

       ssoflux need only be run on the calibrator sources with a known flux
       density and/or model.

       Keyword arguments:
       vis -- Name of input visibility file
       default: none.  example: vis='ngc5921.ms'
       field -- Select field using field id(s) or field name(s).
      default: ''=all fields, but run ssoflux one field at a time.
 [run listobs to obtain the list id's or names of calibrators]
      If field is a non-negative integer, it is assumed to be a field
      index.  Otherwise, it is taken to be a field name.
      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
      default: ''=all spectral windows and channels
      spw='0~2,4'; spectral windows 0,1,2,4 (all channels)
      spw='<2';  spectral windows less than 2 (i.e. 0,1)
      spw='0:5~61'; spw 0, channels 5 to 61
      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;4'; spw 0, channels 0-10,
       spw 1, channels 20-30, and spw 2, channels, 1,2 and 4

       Use one of the two methods below:  modimage or fluxdensity

       modimage -- Model image (I only) for setting the model visibilities.
      default: '' means use fluxdensity instead of modimage. 
      Each field must be done separately.  The image clean model
      will be scaled from the frequency in the model to that actually used,
      unless fluxdensity = 0 (or fluxdensity[0] = 0).
      Both the amplitude and phase are calculated.
      At the AOC or CV, the models are located in
      /usr/lib/casapy/data/nrao/VLA/CalModels/3C286_L.im (egs)
   lib64

       fluxdensity -- Specified flux density [I,Q,U,V] in Jy
       default: -1, uses [1,0,0,0] flux density for all sources,
  except for 3C286, 3C48 and 3C147, which use standard flux
  densities.  It is recommended to use modimage for
  these sources if they are resolved by the observation.
       Only one flux density can be specified at a time.  The phases are
  set to zero.
       example   fluxdensity=-1  will insert 1.0 for all calibrators
         except 3C286, 3C147 and 3C48.
       example   field = '1'; fluxdensity=[3.2,0,0,0] wil put in 
         a flux density of I=3.2 for field='1'

       At present (June 2000), this is the only method to insert a
       polarized flux density model.
       example:  fluxdensity=[2.63,0.21,-0.33,0.02]
         will put in I,Q,U,V flux densities of 2.63,0.21,-0.33,
         and 0.02, respectively, in the model column.

       standard -- Flux density standard, used if fluxdensity<0
       default: 'Perley-Taylor 99'; example: standard='Baars'
       Options: 'Baars','Perley 90','Perley-Taylor 95',
  'Perley-Taylor 99', 'Perley-Butler 2010',
  and 'Butler-JPL-Horizons 2010'.
       All but the last one are for extragalactic calibrators,
       and the final one is for Solar System objects.

Definition at line 46 of file ssoflux_cli.py.

def ssoflux_cli.ssoflux_cli_.check_params	(	self,
		param = `None`,
		value = `None`,
		ipython_globals = `None`
	)

Definition at line 327 of file ssoflux_cli.py.

def ssoflux_cli.ssoflux_cli_.defaults	(	self,
		param = `None`,
		ipython_globals = `None`,
		paramvalue = `None`,
		subparam = `None`
	)

Definition at line 275 of file ssoflux_cli.py.

def ssoflux_cli.ssoflux_cli_.description	(	self,
		key = `'ssoflux'`,
		subkey = `None`
	)

Definition at line 358 of file ssoflux_cli.py.

def ssoflux_cli.ssoflux_cli_.itsdefault	(	self,
		paramname
	)

Definition at line 373 of file ssoflux_cli.py.

Referenced by uvsub_cli.uvsub_cli_.defaults(), uvcontsub2_cli.uvcontsub2_cli_.defaults(), tclean_cli.tclean_cli_.defaults(), testconcat_cli.testconcat_cli_.defaults(), viewer_cli.viewer_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(), virtualconcat_cli.virtualconcat_cli_.defaults(), visstat_cli.visstat_cli_.defaults(), widebandpbcor_cli.widebandpbcor_cli_.defaults(), uvmodelfit_cli.uvmodelfit_cli_.defaults(), statwt_cli.statwt_cli_.defaults(), and widefield_cli.widefield_cli_.defaults().

def ssoflux_cli.ssoflux_cli_.paramgui	(	self,
		useGlobals = `True`,
		ipython_globals = `None`
	)

Opens a parameter GUI for this task.  If useGlobals is true, then any relevant global parameter settings are used.

Definition at line 251 of file ssoflux_cli.py.

def ssoflux_cli.ssoflux_cli_.result	(	self,
		key = `None`
	)

Definition at line 33 of file ssoflux_cli.py.

References accum_cli.accum_cli_.__async__, ssoflux_cli.ssoflux_cli_.__async__, split_cli.split_cli_.__async__, splattotable_cli.splattotable_cli_.__async__, specfit_cli.specfit_cli_.__async__, smoothcal_cli.smoothcal_cli_.__async__, slsearch_cli.slsearch_cli_.__async__, simobserve_cli.simobserve_cli_.__async__, simanalyze_cli.simanalyze_cli_.__async__, simalma_cli.simalma_cli_.__async__, setjy_cli.setjy_cli_.__async__, sdtpimaging_cli.sdtpimaging_cli_.__async__, sdstat_cli.sdstat_cli_.__async__, sdsmooth_cli.sdsmooth_cli_.__async__, sdscale_cli.sdscale_cli_.__async__, sdsave_cli.sdsave_cli_.__async__, sdreduce_cli.sdreduce_cli_.__async__, sdplot_cli.sdplot_cli_.__async__, sdmath_cli.sdmath_cli_.__async__, sdlist_cli.sdlist_cli_.__async__, sdimprocess_cli.sdimprocess_cli_.__async__, sdimaging_cli.sdimaging_cli_.__async__, sdgrid_cli.sdgrid_cli_.__async__, sdflagmanager_cli.sdflagmanager_cli_.__async__, sdflag_cli.sdflag_cli_.__async__, sdfit_cli.sdfit_cli_.__async__, sdcoadd_cli.sdcoadd_cli_.__async__, sdcal_cli.sdcal_cli_.__async__, sdbaseline_cli.sdbaseline_cli_.__async__, rmtables_cli.rmtables_cli_.__async__, predictcomp_cli.predictcomp_cli_.__async__, polcal_cli.polcal_cli_.__async__, plotxy_cli.plotxy_cli_.__async__, plotweather_cli.plotweather_cli_.__async__, plotuv_cli.plotuv_cli_.__async__, plotms_cli.plotms_cli_.__async__, plotcal_cli.plotcal_cli_.__async__, plotants_cli.plotants_cli_.__async__, peel_cli.peel_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__.

Member Data Documentation

dictionary ssoflux_cli.ssoflux_cli_.__async__ [static, private]

Definition at line 20 of file ssoflux_cli.py.

Referenced by ssoflux_cli.ssoflux_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(), and statwt_cli.statwt_cli_.result().

ssoflux_cli.ssoflux_cli_.__bases__ [private]

Definition at line 27 of file ssoflux_cli.py.

ssoflux_cli.ssoflux_cli_.__doc__ [private]

Definition at line 28 of file ssoflux_cli.py.

ssoflux_cli.ssoflux_cli_.__globals__ [private]

Definition at line 136 of file ssoflux_cli.py.

string ssoflux_cli.ssoflux_cli_.__name__ [static, private]

Definition at line 19 of file ssoflux_cli.py.

ssoflux_cli.ssoflux_cli_.i_am_a_casapy_task [static]

Definition at line 22 of file ssoflux_cli.py.

ssoflux_cli.ssoflux_cli_.parameters

Definition at line 30 of file ssoflux_cli.py.

Referenced by tclean_cli.tclean_cli_.itsdefault(), vishead_cli.vishead_cli_.itsdefault(), wvrgcal_cli.wvrgcal_cli_.itsdefault(), widebandpbcor_cli.widebandpbcor_cli_.itsdefault(), visstat_cli.visstat_cli_.itsdefault(), uvmodelfit_cli.uvmodelfit_cli_.itsdefault(), statwt_cli.statwt_cli_.itsdefault(), and widefield_cli.widefield_cli_.itsdefault().

tuple ssoflux_cli.ssoflux_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 306 of file ssoflux_cli.py.

tuple ssoflux_cli.ssoflux_cli_.retval [static]

Definition at line 319 of file ssoflux_cli.py.

ssoflux_cli.ssoflux_cli_.rkey [static]

Handle globals or user over-ride of arguments.

Definition at line 21 of file ssoflux_cli.py.

string ssoflux_cli.ssoflux_cli_.valornotval [static]

Definition at line 309 of file ssoflux_cli.py.

The documentation for this class was generated from the following file:

ssoflux_cli.py

Public Member Functions

Public Attributes

Static Public Attributes

Private Attributes

Static Private Attributes

Detailed Description

Constructor & Destructor Documentation

Member Function Documentation

Member Data Documentation