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<ri:Resource created="2024-07-01T08:03:17Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>MeerKAT calibrator sources polarization properties</title><shortName>J/AJ/167/273</shortName><identifier>ivo://CDS.VizieR/J/AJ/167/273</identifier><altIdentifier>doi:10.26093/cds/vizier.51670273</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Taylor A.R.</name></creator><creator><name>Legodi L.S.</name></creator><date role="Updated">2024-11-06T20:20:20Z</date><date role="Created">2024-07-01T08:03:17Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>radio-continuum-emission</subject><subject>interferometry</subject><subject>active-galactic-nuclei</subject><description>We report on full-Stokes L-band observations of 98 MeerKAT calibration sources. Linear polarization is detected in 71 objects above a fractional level of 0.2%. We identify ten sources with strong fractional linear polarization and low Faraday rotation measure that could be suitable for wide-band absolute polarization calibration. We detect significant circular polarization from 24% of the sample down to a detection level of 0.07%. Circularly polarized emission is seen only for flat spectrum sources {alpha}&gt;-0.5. We compare our polarized intensities and Faraday synthesis results to data from the NVSS at 1400MHz and the ATCA SPASS survey at 2300MHz. NVSS data exist for 54 of our sources and SPASS data for 20 sources. The percent polarization and rotation measures from both surveys agree well with our results. The residual instrumental linear polarization for these observations is measured at 0.16%, and the residual instrumental circular polarization is measured at 0.05%. These levels may reflect either instabilities in the relative bandpass between the two polarization channels with either time or antenna orientation, or atmospheric/ionospheric variations with pointing direction. Tracking of the hourly gain solutions on J0408-6545 after transfer of the primary gain solutions suggests a deterioration of the gain stability by a factor of several starting about 2hr after sunrise. This suggests that observing during the nighttime could dramatically improve the precision of polarization calibration.</description><source format="bibcode">2024AJ....167..273T</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/167/273</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/VII/2">VII/2 : Master list of radio sources, updated 1978 (Dixon, 1970)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VIII/38">VIII/38 : The Parkes-MIT-NRAO 4.85GHz (PMN) Surveys (Griffith+ 1993-1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VIII/65">VIII/65 : 1.4GHz NRAO VLA Sky Survey (NVSS) (Condon+ 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VIII/74">VIII/74 : SPECFIND Catalog of radio continuum spectra (Vollmer+ 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VIII/85">VIII/85 : SPECFIND V2.0 Catalog of radio continuum spectra (Vollmer+ 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/702/1230">J/ApJ/702/1230 : Rotation measure image of the sky (Taylor+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/212/15">J/ApJS/212/15 : Polarized NVSS sources SEDs (Farnes+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/829/5">J/ApJ/829/5 : SPASS &amp; NVSS bright extragalactic radio sources (Lamee+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/PASA/34.13">J/other/PASA/34.13 : S-PASS catalog at 2.3GHz (Meyers+, 2017)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/AJ/167/273</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/167/273</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/167/273</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/167/273</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/167/273</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/167/273</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><coverage><footprint ivo-id="ivo://ivoa.net/std/moc"/><waveband>Radio</waveband></coverage><tableset><schema><name>default</name><table><name>J/AJ/167/273/table3</name><description>Polarization properties of MeerKAT calibrator sources</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>S1.4GHz</name><description>[0.52/16.2] Flux density at 1400MHz from a power-law fit to the Stokes I spectrum (1)</description><unit>Jy</unit><ucd>phot.flux.density;em.radio.750-1500MHz</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_S1.4GHz</name><description>[0.001/0.02] Uncertainty in S1.4GHz (1)</description><unit>Jy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>alpha</name><description>[-1.31/1.48] In-band spectral index, Equation 11 (1)</description><ucd>spect.index</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_alpha</name><description>[0.001/0.02] Uncertainty in alpha (1)</description><ucd>stat.error;spect.index</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>C</name><description>[-0.83/0.68] Curvature term from spectral fit to the Stokes I spectrum</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_C</name><description>[0.003/0.04] Uncertainty in C</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>p1400</name><description>[0.01/9.9] Percent polarized intensity at 1400MHz (2)</description><unit>%</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_p1400</name><description>[0.0/0.013] Uncertainty in p1400 (2)</description><unit>%</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>PA1400</name><description>[-86.5/84.8] Position angle at 1400 MHz (2)</description><unit>deg</unit><ucd>pos.posAng</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_PA1400</name><description>[0.1/21.7] Uncertainty in PA1400 (2)</description><unit>deg</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>beta</name><description>[-7.37/3.25] Spectral index of polarized intensity (3)</description><ucd>spect.index</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_beta</name><description>[0.01/0.34] Uncertainty in beta (3)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RM</name><description>[-127/107] Faraday depth of dominant rotation measure synthesis component</description><unit>rad.m**-2</unit><ucd>phys.veloc.rotat</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_RM</name><description>[0.1/2] Uncertainty in RM</description><unit>rad.m**-2</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>pmax</name><description>[0.02/9.39] Amplitude (percent polarization) of dominant rotation measure synthesis component</description><unit>%</unit><ucd>src.var.amplitude</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_vmed</name><description>[0.001/0.003] Uncertainty in vmed (4)</description><unit>%</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>vmed</name><description>[-0.23/0.36] Median value fractional Stokes V over the band (4)</description><unit>%</unit><ucd>phys.polarization.stokes;stat.median</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>v1400</name><description>[-0.22/0.31] Circular polarization at 1400MHz from spectral fit to v spectrum</description><unit>%</unit><ucd>phys.polarization.circular</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_v1400</name><description>[0.001/0.02] Uncertainty in v1400</description><unit>%</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Name</name><description>J2000-based source name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column></table></schema></tableset></ri:Resource>