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 fixplanets_cli.py.

Constructor & Destructor Documentation

def fixplanets_cli.fixplanets_cli_.__init__ ( self )

Definition at line 26 of file fixplanets_cli.py.

Member Function Documentation

def fixplanets_cli.fixplanets_cli_.__call__	(	self,
		vis = `None`,
		field = `None`,
		fixuvw = `None`,
		direction = `None`,
		refant = `None`,
		reftime = `None`,
		async = `None`
	)

Changes FIELD and SOURCE table entries based on user given direction or POINTING table, optionally fixes the UVW coordinates
    This task's main purpose is to correct observations which were performed
    with correct pointing and correlation but for which incorrect direction
    information was entered in the FIELD and SOURCE table of the MS.
    If you actually want to change the phase center of the visibilties in an MS,
    you should use task fixvis.

    Input Parameters
    vis        -- Name of the input visibility set
    
    field      -- field selection string
    
    fixuvw     -- recalc uvw coordinates? (default: False)

    direction  -- if set, don't use pointing table but set direction to this value
  default= '' (use pointing table)
  example: 'J2000 19h30m00 -40d00m00'

    refant     -- if using pointing table information, use it from this antenna
  default: 0 (antenna id 0)
  examples: 'DV06' (antenna with name DV06)
            3 (antenna id 3)
    reftime    -- if using pointing table information, use it from this timestamp
  default: 'first'
  examples: 'median' will use the median timestamp for the given field
            using only the unflagged maintable rows 
            '2012/07/11/08:41:32' will use the given timestamp (must be
            within the observaton time)

    Examples:

    fixplanets('uid___A002_X1c6e54_X223.ms', 'Titan', True)
  will look up the pointing direction from antenna 0 for field 'Titan' in 
  the POINTING table based on the first timestamp in the main table rows for 
  this field, enter this direction in the FIELD and SOURCE tables, and then 
  recalculate the UVW coordinates for this field.

    fixplanets('uid___A002_X1c6e54_X223.ms', 'Titan', False, 'J2000 12h30m15 -02d12m00')
  will set the directions for field 'Titan' in the FIELD and SOURCE table to the
  given direction and not recalculate the UVW coordinates.
  (This can be useful for several purposes, among them preparing a concatenation
  of datasets. Only fields with the same direction will be recognised as identical.
  fixplanets can then be run again after the concatenation using parameters as in
  the first example above.)

Definition at line 46 of file fixplanets_cli.py.

def fixplanets_cli.fixplanets_cli_.check_params	(	self,
		param = `None`,
		value = `None`,
		ipython_globals = `None`
	)

Definition at line 286 of file fixplanets_cli.py.

References clearstat_cli.clearstat_cli_.__globals__, clearplot_cli.clearplot_cli_.__globals__, find_cli.find_cli_.__globals__, asdmsummary_cli.asdmsummary_cli_.__globals__, conjugatevis_cli.conjugatevis_cli_.__globals__, delmod_cli.delmod_cli_.__globals__, exportfits_cli.exportfits_cli_.__globals__, caltabconvert_cli.caltabconvert_cli_.__globals__, boxit_cli.boxit_cli_.__globals__, calstat_cli.calstat_cli_.__globals__, deconvolve_cli.deconvolve_cli_.__globals__, clearcal_cli.clearcal_cli_.__globals__, fixplanets_cli.fixplanets_cli_.__globals__, exportasdm_cli.exportasdm_cli_.__globals__, browsetable_cli.browsetable_cli_.__globals__, feather_cli.feather_cli_.__globals__, exportuvfits_cli.exportuvfits_cli_.__globals__, concat_cli.concat_cli_.__globals__, csvclean_cli.csvclean_cli_.__globals__, accum_cli.accum_cli_.__globals__, blcal_cli.blcal_cli_.__globals__, applycal_cli.applycal_cli_.__globals__, cvel_cli.cvel_cli_.__globals__, bandpass_cli.bandpass_cli_.__globals__, autoclean_cli.autoclean_cli_.__globals__, and clean_cli.clean_cli_.__globals__.

def fixplanets_cli.fixplanets_cli_.defaults	(	self,
		param = `None`,
		ipython_globals = `None`,
		paramvalue = `None`,
		subparam = `None`
	)

Definition at line 234 of file fixplanets_cli.py.

def fixplanets_cli.fixplanets_cli_.description	(	self,
		key = `'fixplanets'`,
		subkey = `None`
	)

Definition at line 317 of file fixplanets_cli.py.

def fixplanets_cli.fixplanets_cli_.itsdefault	(	self,
		paramname
	)

Definition at line 332 of file fixplanets_cli.py.

Referenced by rmtables_cli.rmtables_cli_.defaults(), listfits_cli.listfits_cli_.defaults(), listhistory_cli.listhistory_cli_.defaults(), importfitsidi_cli.importfitsidi_cli_.defaults(), uvsub_cli.uvsub_cli_.defaults(), uvcontsub2_cli.uvcontsub2_cli_.defaults(), importgmrt_cli.importgmrt_cli_.defaults(), plotweather_cli.plotweather_cli_.defaults(), importuvfits_cli.importuvfits_cli_.defaults(), plotants_cli.plotants_cli_.defaults(), imreframe_cli.imreframe_cli_.defaults(), importfits_cli.importfits_cli_.defaults(), smoothcal_cli.smoothcal_cli_.defaults(), listsdm_cli.listsdm_cli_.defaults(), tclean_cli.tclean_cli_.defaults(), splattotable_cli.splattotable_cli_.defaults(), hanningsmooth_cli.hanningsmooth_cli_.defaults(), flagmanager_cli.flagmanager_cli_.defaults(), sdflagmanager_cli.sdflagmanager_cli_.defaults(), testconcat_cli.testconcat_cli_.defaults(), sdlist_cli.sdlist_cli_.defaults(), msview_cli.msview_cli_.defaults(), fixplanets_cli.fixplanets_cli_.defaults(), viewer_cli.viewer_cli_.defaults(), fixvis_cli.fixvis_cli_.defaults(), imregrid_cli.imregrid_cli_.defaults(), listpartition_cli.listpartition_cli_.defaults(), sdscale_cli.sdscale_cli_.defaults(), imsubimage_cli.imsubimage_cli_.defaults(), ft_cli.ft_cli_.defaults(), msmoments_cli.msmoments_cli_.defaults(), impbcor_cli.impbcor_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(), listobs_cli.listobs_cli_.defaults(), sdsmooth_cli.sdsmooth_cli_.defaults(), fluxscale_cli.fluxscale_cli_.defaults(), visstat_cli.visstat_cli_.defaults(), imview_cli.imview_cli_.defaults(), widebandpbcor_cli.widebandpbcor_cli_.defaults(), sdcoadd_cli.sdcoadd_cli_.defaults(), uvmodelfit_cli.uvmodelfit_cli_.defaults(), listvis_cli.listvis_cli_.defaults(), sdsave_cli.sdsave_cli_.defaults(), simanalyze_cli.simanalyze_cli_.defaults(), imhead_cli.imhead_cli_.defaults(), sdmath_cli.sdmath_cli_.defaults(), listcal_cli.listcal_cli_.defaults(), sdgrid_cli.sdgrid_cli_.defaults(), importasdm_cli.importasdm_cli_.defaults(), sdtpimaging_cli.sdtpimaging_cli_.defaults(), sdstat_cli.sdstat_cli_.defaults(), makemask_cli.makemask_cli_.defaults(), split_cli.split_cli_.defaults(), sdimaging_cli.sdimaging_cli_.defaults(), statwt_cli.statwt_cli_.defaults(), sdflag_cli.sdflag_cli_.defaults(), importevla_cli.importevla_cli_.defaults(), partition_cli.partition_cli_.defaults(), simalma_cli.simalma_cli_.defaults(), imfit_cli.imfit_cli_.defaults(), sdfit_cli.sdfit_cli_.defaults(), sdcal_cli.sdcal_cli_.defaults(), simobserve_cli.simobserve_cli_.defaults(), gaincal_cli.gaincal_cli_.defaults(), polcal_cli.polcal_cli_.defaults(), sdbaseline_cli.sdbaseline_cli_.defaults(), setjy_cli.setjy_cli_.defaults(), mosaic_cli.mosaic_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(), sdreduce_cli.sdreduce_cli_.defaults(), flagcmd_cli.flagcmd_cli_.defaults(), and flagdata_cli.flagdata_cli_.defaults().

def fixplanets_cli.fixplanets_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 210 of file fixplanets_cli.py.

References clearstat_cli.clearstat_cli_.__globals__, clearplot_cli.clearplot_cli_.__globals__, find_cli.find_cli_.__globals__, asdmsummary_cli.asdmsummary_cli_.__globals__, conjugatevis_cli.conjugatevis_cli_.__globals__, delmod_cli.delmod_cli_.__globals__, exportfits_cli.exportfits_cli_.__globals__, caltabconvert_cli.caltabconvert_cli_.__globals__, boxit_cli.boxit_cli_.__globals__, calstat_cli.calstat_cli_.__globals__, deconvolve_cli.deconvolve_cli_.__globals__, clearcal_cli.clearcal_cli_.__globals__, fixplanets_cli.fixplanets_cli_.__globals__, exportasdm_cli.exportasdm_cli_.__globals__, browsetable_cli.browsetable_cli_.__globals__, feather_cli.feather_cli_.__globals__, exportuvfits_cli.exportuvfits_cli_.__globals__, concat_cli.concat_cli_.__globals__, csvclean_cli.csvclean_cli_.__globals__, accum_cli.accum_cli_.__globals__, blcal_cli.blcal_cli_.__globals__, applycal_cli.applycal_cli_.__globals__, cvel_cli.cvel_cli_.__globals__, bandpass_cli.bandpass_cli_.__globals__, autoclean_cli.autoclean_cli_.__globals__, and clean_cli.clean_cli_.__globals__.

def fixplanets_cli.fixplanets_cli_.result	(	self,
		key = `None`
	)

Definition at line 33 of file fixplanets_cli.py.

References accum_cli.accum_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 fixplanets_cli.fixplanets_cli_.__async__ [static, private]

Definition at line 20 of file fixplanets_cli.py.

Referenced by fixplanets_cli.fixplanets_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(), peel_cli.peel_cli_.result(), pclean_cli.pclean_cli_.result(), partition_cli.partition_cli_.result(), msview_cli.msview_cli_.result(), msmoments_cli.msmoments_cli_.result(), mosaic_cli.mosaic_cli_.result(), makemask_cli.makemask_cli_.result(), listvis_cli.listvis_cli_.result(), listsdm_cli.listsdm_cli_.result(), listpartition_cli.listpartition_cli_.result(), listobs_cli.listobs_cli_.result(), listhistory_cli.listhistory_cli_.result(), listfits_cli.listfits_cli_.result(), listcal_cli.listcal_cli_.result(), imview_cli.imview_cli_.result(), imval_cli.imval_cli_.result(), imtrans_cli.imtrans_cli_.result(), imsubimage_cli.imsubimage_cli_.result(), imstat_cli.imstat_cli_.result(), imsmooth_cli.imsmooth_cli_.result(), imregrid_cli.imregrid_cli_.result(), imreframe_cli.imreframe_cli_.result(), importvla_cli.importvla_cli_.result(), importuvfits_cli.importuvfits_cli_.result(), importgmrt_cli.importgmrt_cli_.result(), importfitsidi_cli.importfitsidi_cli_.result(), importfits_cli.importfits_cli_.result(), importevla_cli.importevla_cli_.result(), importasdm_cli.importasdm_cli_.result(), impbcor_cli.impbcor_cli_.result(), immoments_cli.immoments_cli_.result(), immath_cli.immath_cli_.result(), imhead_cli.imhead_cli_.result(), imfit_cli.imfit_cli_.result(), imcontsub_cli.imcontsub_cli_.result(), imcollapse_cli.imcollapse_cli_.result(), hanningsmooth_cli.hanningsmooth_cli_.result(), gencal_cli.gencal_cli_.result(), gaincal_cli.gaincal_cli_.result(), ft_cli.ft_cli_.result(), fluxscale_cli.fluxscale_cli_.result(), flagmanager_cli.flagmanager_cli_.result(), flagdata_cli.flagdata_cli_.result(), flagcmd_cli.flagcmd_cli_.result(), and fixvis_cli.fixvis_cli_.result().

fixplanets_cli.fixplanets_cli_.__bases__ [private]

Definition at line 27 of file fixplanets_cli.py.

fixplanets_cli.fixplanets_cli_.__doc__ [private]

Definition at line 28 of file fixplanets_cli.py.

fixplanets_cli.fixplanets_cli_.__globals__ [private]

Definition at line 95 of file fixplanets_cli.py.

string fixplanets_cli.fixplanets_cli_.__name__ [static, private]

Definition at line 19 of file fixplanets_cli.py.

fixplanets_cli.fixplanets_cli_.i_am_a_casapy_task [static]

Definition at line 22 of file fixplanets_cli.py.

fixplanets_cli.fixplanets_cli_.parameters

Definition at line 30 of file fixplanets_cli.py.

tuple fixplanets_cli.fixplanets_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 265 of file fixplanets_cli.py.

tuple fixplanets_cli.fixplanets_cli_.retval [static]

Definition at line 278 of file fixplanets_cli.py.

fixplanets_cli.fixplanets_cli_.rkey [static]

Handle globals or user over-ride of arguments.

Definition at line 21 of file fixplanets_cli.py.

string fixplanets_cli.fixplanets_cli_.valornotval [static]

Definition at line 268 of file fixplanets_cli.py.

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

fixplanets_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