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<casaxml xsi:schemaLocation="http://casa.nrao.edu/schema/casa.xsd file:///opt/casa/code/xmlcasa/xml/casa.xsd" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns="http://casa.nrao.edu/schema/psetTypes.html">
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<task category="manipulation" name="testconcat" type="function">
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<shortdescription>Concatenate the subtables of several visibility data sets, not the MAIN bulk data.</shortdescription>
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<input>
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<param mustexist="true" name="vis" type="pathVec">
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<description>Name(s) of input visibility files to be test-concatenated</description>
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<value/>
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</param>
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<param name="testconcatvis" type="string">
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<description>Name of output MS containing the merged subtables</description>
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<value/>
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</param>
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<param name="freqtol" type="any">
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<description>Frequency shift tolerance for considering data as the same spwid</description>
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<any type="variant"/>
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<value type="string"/>
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</param>
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<param name="dirtol" type="any">
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<description>Direction shift tolerance for considering data as the same field</description>
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<any type="variant"/>
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<value type="string"/>
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</param>
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<param name="copypointing" type="bool">
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<description>Copy all rows of the POINTING table.</description>
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<value>True</value>
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</param>
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</input>
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<example>
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The list of data sets given in the vis argument are concatenated into an output
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data set in testconcatvis without the bulk data of the MAIN table.
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This is useful for obtaining the information in the merged subtables without
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actually performing a time-consuming concatenation of the MAIN tables on disk.
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Keyword arguments:
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vis -- Name of input visibility files for which the subtables are to be combined
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default: none; example: vis = 'mydata.ms',
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vis=['src2.ms','ngc5921.ms','ngc315.ms']
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testconcatvis -- Name of MS that will contain the concatenated subtables
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default: none; example: testconcatvis='test.ms'
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freqtol -- Frequency shift tolerance for considering data to be in the same
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spwid. The number of channels must also be the same.
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default: '' do not combine unless frequencies are equal
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example: freqtol='10MHz' will not combine spwid unless they are
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within 10 MHz.
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Note: This option is useful to conbine spectral windows with very slight
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frequency differences caused by Doppler tracking, for example.
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dirtol -- Direction shift tolerance for considering data as the same field
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default: '' means always combine.
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example: dirtol='1.arcsec' will not combine data for a field unless
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their phase center differ by less than 1 arcsec. If the field names
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are different in the input data sets, the name in the output data
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set will be the first relevant data set in the list.
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copypointing -- Make a proper copy of the POINTING subtable (can be time consuming).
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If False, the result is an empty POINTING table.
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default: True
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</example>
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<returns>void</returns></task>
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</casaxml>