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importuvfits_pg.importuvfits_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 importuvfits_pg.py.


Constructor & Destructor Documentation

Definition at line 21 of file importuvfits_pg.py.


Member Function Documentation

def importuvfits_pg.importuvfits_pg_.__call__ (   self,
  fitsfile = None,
  vis = None,
  antnamescheme = None,
  async = None 
)
Convert a UVFITS file to a CASA visibility data set
Convert a UVFITS file to a CASA visibility data set:

Keyword arguments:
fitsfile -- Name of input UV FITS file
default = none; example='3C273XC1.fits'
vis -- Name of output visibility file (MS)
default = none; example: vis='3C273XC1.ms'
antnamescheme -- Naming scheme for VLA/JVLA/CARMA antennas
default = old;
  old: Antenna name is a number, '04'
       This option exists for backwards compatibility
       but can lead to ambiguous results when antenna
       indices are used for data selection.
  new: Antenna name is not a number, e.g., 'VA04' or 'EA04'
       With this scheme, data selection via
       antenna names and indices is non-ambiguous.
async --  Run asynchronously
       default = false; do not run asychronously

Note: Don't forget to flag autocorrections using
   taskname flagdata, autocorr = true

Definition at line 26 of file importuvfits_pg.py.

References vla_uvfits_line_sf.verify.


Member Data Documentation

Definition at line 22 of file importuvfits_pg.py.

Definition at line 23 of file importuvfits_pg.py.

Definition at line 19 of file importuvfits_pg.py.


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