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ft_pg.ft_pg_ Class Reference

List of all members.

Public Member Functions

def __init__
def __call__

Private Attributes

 __bases__
 __doc__

Static Private Attributes

string __name__

Detailed Description

Definition at line 18 of file ft_pg.py.


Constructor & Destructor Documentation

def ft_pg.ft_pg_.__init__ (   self)

Definition at line 21 of file ft_pg.py.


Member Function Documentation

def ft_pg.ft_pg_.__call__ (   self,
  vis = None,
  field = None,
  spw = None,
  model = None,
  nterms = None,
  reffreq = None,
  complist = None,
  incremental = None,
  usescratch = None,
  async = None 
)
Insert a source model  a visibility set:

       A source model (souce.model image) or components list is converted into a
       model visibility that is inserted into the MODEL_DATA column.  This is
       needed to use resolved source in gaincal and in fluxscale.  

       Setjy will automatically make this ft step on the
       sources currently available are 3C48, 3C138, 3C147, 3C286
       at 1.4, 5.0, 8.4, 15, 22, 43 GHz.  Their location is site
       dependent.  In Charlottesville and at the AOC, the models are
       in /usr/lib(lib64)/casapy/data/nrao/VLA/CalModels.
       

       Keyword arguments:
       vis -- Name of input visibility file
      default: none; example: vis='ngc5921.ms'
       field -- Field name list
       default: '' ==> all
       NOTE: BUT, only one source can be specified in a multi-source vis.
       field = '1328+307'  specifies source '1328+307'
       field = '4' specified field with index 4
       spw -- Spw selection
       default: spw = '' (all spw)
       model -- Name of input model image
       default: '' ==> None;
       example: model='/usr/lib/casapy/data/nrao/VLA/CalModels/3C286_X.im'
       Note: The model visibilities are scaled from the model frequency
     to the observed frequency of the data.
       nterms -- Number of terms used to model the sky frequency dependence
 default: 1  ==> one model image is required
 example : nterms=3  represents a 2nd order Taylor-polynomial in frequency
           and should be used in conjuction with coefficient model images as 
           model=['xxx.model.tt0','xxx.model.tt1', 'xxx.model.tt2']
     reffreq -- Reference-frequency about which this Taylor-expansion is defined.
        default: '' ==> reads the reference frequency from the model image
        example : reffreq = '1.5GHz'
       complist -- Name of component list
       default: None; ; example: complist='test.cl'
       component lists are difficult to make.
       incremental -- Add model visibility to the existing model visibilties stored in the MS
       default: False; example: incremental=True
       usescratch  -- if True model visibilities will be stored in the scratch column 
            MODEL_DATA; when false the model visibilities will be generated 
            on the fly (this mode may save some disk space equivalent to 
            the volume of the observed data). 
            default: False; example usescratch=True

Definition at line 26 of file ft_pg.py.

References vla_uvfits_line_sf.verify.


Member Data Documentation

Definition at line 22 of file ft_pg.py.

Definition at line 23 of file ft_pg.py.

string ft_pg.ft_pg_.__name__ [static, private]

Definition at line 19 of file ft_pg.py.


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