Public Member Functions | |
def | __init__ |
def | __call__ |
Private Attributes | |
__bases__ | |
__doc__ | |
Static Private Attributes | |
string | __name__ |
Definition at line 18 of file importuvfits_pg.py.
def importuvfits_pg.importuvfits_pg_.__init__ | ( | self | ) |
Definition at line 21 of file importuvfits_pg.py.
def importuvfits_pg.importuvfits_pg_.__call__ | ( | self, | |
fitsfile = None , |
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vis = None , |
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antnamescheme = None , |
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async = None |
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) |
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.
Definition at line 22 of file importuvfits_pg.py.
importuvfits_pg.importuvfits_pg_.__doc__ [private] |
Definition at line 23 of file importuvfits_pg.py.
string importuvfits_pg.importuvfits_pg_.__name__ [static, private] |
Definition at line 19 of file importuvfits_pg.py.