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__ |
Proxy of C++ casac::vlafillertask class
Definition at line 70 of file vlafillertask.py.
def __casac__.vlafillertask.vlafillertask.__init__ | ( | self | ) |
__init__(self) -> vlafillertask
Definition at line 77 of file vlafillertask.py.
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 --------------------------------------------------------------------------------
Definition at line 84 of file vlafillertask.py.
__casac__.vlafillertask.vlafillertask.__del__ [static, private] |
Definition at line 83 of file vlafillertask.py.
tuple __casac__.vlafillertask.vlafillertask.__getattr__ [static, private] |
Definition at line 75 of file vlafillertask.py.
__casac__.vlafillertask.vlafillertask.__repr__ [static, private] |
Definition at line 76 of file vlafillertask.py.
tuple __casac__.vlafillertask.vlafillertask.__setattr__ [static, private] |
Definition at line 73 of file vlafillertask.py.
__casac__.vlafillertask.vlafillertask.__swig_destroy__ [static, private] |
Definition at line 82 of file vlafillertask.py.
dictionary __casac__.vlafillertask.vlafillertask.__swig_getmethods__ [static, private] |
Definition at line 74 of file vlafillertask.py.
dictionary __casac__.vlafillertask.vlafillertask.__swig_setmethods__ [static, private] |
Definition at line 72 of file vlafillertask.py.
Definition at line 81 of file vlafillertask.py.