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__casac__.vlafillertask.vlafillertask Class Reference
Inheritance diagram for __casac__.vlafillertask.vlafillertask:
__casac__.vlafillertask._object

List of all members.

Public Member Functions

def __init__
def fill

Public Attributes

 this

Static Private Attributes

dictionary __swig_setmethods__
tuple __setattr__
dictionary __swig_getmethods__
tuple __getattr__
 __repr__
 __swig_destroy__
 __del__

Detailed Description

Proxy of C++ casac::vlafillertask class

Definition at line 70 of file vlafillertask.py.


Constructor & Destructor Documentation

__init__(self) -> vlafillertask

Definition at line 77 of file vlafillertask.py.


Member Function Documentation

def __casac__.vlafillertask.vlafillertask.fill (   self,
  args,
  kwargs 
)
fill(self, msname, inputfile, project=string(""), start=string("1970/1/1/00:00:00"), stop=string("2199/1/1/23:59:59"), 
    centerfreq=string("1.0e18Hz"), bandwidth=string("2.0e18Hz"), 
    bandname=string("*"), source=string(""), subarray=0, qualifier=-65536, 
    calcode=string("#"), overwrite=False, freqtol=initialize_variant("0.0"), 
    applytsys=True, keepautocorr=False, antnamescheme=string("new"), useday=1, 
    keepblanks=False, evlabands=True)

Summary
Perform fill operations

Input Parameters:
msname           name of output ms 
inputfile        name of vla archive 
project          name of project to extract, defaults to all projects in input 
start            start time to extract 1970/1/1/00:00:00 
stop             end time of extracted data 2199/1/1/23:59:59 
centerfreq       frequency of data to extract (used along with bandwidth param) 1.0e18Hz 
bandwidth        data around centerfreq to get out 2.0e18Hz 
bandname         name of band to extract 4 P L C X U K Q * 
source           name of source 
subarray         subarray - 0 means all subarrays 0 
qualifier        qualifier for source -65536 
calcode          Calibrator code, 1 character only * # 
overwrite        overwrite or append false 
freqtol          Frequency tolerance, the default tolerance for frequency is set to be 6 times of the channel width. You may have to tweak the tolerance depending on the dataset, just depends. 0.0 
applytsys        scale data and weights by Tsys info true 
keepautocorr     Fill autocorrelations along with cross correlation data. If False data that have same ANTENNA1 and ANTENNA2 are ignored false 
antnamescheme    If 'new', VLA antenna name is prepended by EVLA or VLA to distinguish between the refurbished and non-refubished antennas. 'old' will just put the VLA antenna identifier as is in the NAME column of the ANTENNA table. old new 
useday           This option is only available at the AOC in Socorro! When filling at the AOC, select the online day file to use < 0 means any previous day up to 14 0 means from the start of the current day > 0 means starting now 1 
keepblanks       Scans with blank (empty) source names (i.e. tipping scans) will be filled. The default is to not fill. false 
evlabands        Use the EVLA frequencies and bandwith tolerances when specifying band codes or wavelengths. true 

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Definition at line 84 of file vlafillertask.py.


Member Data Documentation

Definition at line 83 of file vlafillertask.py.

Definition at line 75 of file vlafillertask.py.

Definition at line 76 of file vlafillertask.py.

Definition at line 73 of file vlafillertask.py.

Definition at line 82 of file vlafillertask.py.

Definition at line 74 of file vlafillertask.py.

Definition at line 72 of file vlafillertask.py.

Definition at line 81 of file vlafillertask.py.


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