imreframe_pg.imreframe_pg_ Class Reference

List of all members.

Public Member Functions
def	__init__
def	__call__
Private Attributes
	__bases__
	__doc__
Static Private Attributes
string	__name__

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Detailed Description

Definition at line 18 of file imreframe_pg.py.

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Constructor & Destructor Documentation

def imreframe_pg.imreframe_pg_.__init__

(

self

)

Definition at line 21 of file imreframe_pg.py.

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Member Function Documentation

def imreframe_pg.imreframe_pg_.__call__	(		self,
			imagename = None,
			output = None,
			outframe = None,
			epoch = None,
			restfreq = None,
			async = None
	)

Change the frame in which the image reports its spectral values

    imagename -- name of casa image file to process on
    output         -- name of output image  '' means modify the input image itself
 default: '';           
    outframe     -- new spectral frame in which the frequency or 
                  velocity will be reported for.  
 Options: 'lsrk','lsrd','bary','geo','topo','galacto',
          'lgroup','cmb'
 default: 'lsrk'
    >>> 
 epoch    -- when outframe is 'topo' or 'geo' a time in UTC is needed
                 to decide when to do the frequency conversion. '' is to use 
                 the epoch of the input image
       default= '' 

    restfreq -- Specify rest frequency to use for output image
       default=''; '' means use the restfrequency already in input image
       For example for
       NH_3 (1,1) put restfreq='23.694496GHz'

Definition at line 26 of file imreframe_pg.py.

References vla_uvfits_line_sf.verify.

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Member Data Documentation

imreframe_pg.imreframe_pg_.__bases__ [private]

Definition at line 22 of file imreframe_pg.py.

imreframe_pg.imreframe_pg_.__doc__ [private]

Definition at line 23 of file imreframe_pg.py.

string imreframe_pg.imreframe_pg_.__name__ [static, private]

Definition at line 19 of file imreframe_pg.py.

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

• imreframe_pg.py