Functions | |
def | testconcat |
def testconcat.testconcat | ( | vis = [''] , |
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testconcatvis = '' , |
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freqtol = '' , |
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dirtol = '' , |
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copypointing = True |
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) |
Concatenate the subtables of several visibility data sets, not the MAIN bulk data. The list of data sets given in the vis argument are concatenated into an output data set in testconcatvis without the bulk data of the MAIN table. This is useful for obtaining the information in the merged subtables without actually performing a time-consuming concatenation of the MAIN tables on disk. Keyword arguments: vis -- Name of input visibility files for which the subtables are to be combined default: none; example: vis = 'mydata.ms', vis=['src2.ms','ngc5921.ms','ngc315.ms'] testconcatvis -- Name of MS that will contain the concatenated subtables default: none; example: testconcatvis='test.ms' freqtol -- Frequency shift tolerance for considering data to be in the same spwid. The number of channels must also be the same. default: '' do not combine unless frequencies are equal example: freqtol='10MHz' will not combine spwid unless they are within 10 MHz. Note: This option is useful to conbine spectral windows with very slight frequency differences caused by Doppler tracking, for example. dirtol -- Direction shift tolerance for considering data as the same field default: '' means always combine. example: dirtol='1.arcsec' will not combine data for a field unless their phase center differ by less than 1 arcsec. If the field names are different in the input data sets, the name in the output data set will be the first relevant data set in the list. copypointing -- Make a proper copy of the POINTING subtable (can be time consuming). If False, the result is an empty POINTING table. default: True
Definition at line 13 of file testconcat.py.
References task_testconcat.testconcat(), and vla_uvfits_line_sf.verify.