<?xml version='1.0'?><?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?><ri:Resource created="2016-03-21T21:00:00" status="active" updated="2025-04-11T15:19:14" 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/RegistryInterface/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/RegistryInterface-v1.0.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource-v1.1.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService-v1.1.xsd" xsi:type="vs:CatalogService"><title>LBCS Calibrator Search</title><shortName>LBCS Calibrator Search</shortName><identifier>ivo://astron.nl/lbcs/lobos/cone</identifier><curation><publisher>ASTRON</publisher><creator><name>Deller, A.</name></creator><date role="updated">2025-04-11T15:19:14</date><contact><name>Michael Sipior</name><address>Oude Hoogeveensedijk 4, 7991PD Dwingeloo, the Netherlands</address><email>vo@astron.nl</email></contact></curation><content><subject>Catalogs</subject><description> This service queries the catalog of calibrators from the LOFAR
Long-Baseline Calibrator Survey (LBCS). The LBCS aims to identify
sources suitable for calibrating the highest-resolution observations
made with the International LOFAR Telescope, which include baselines
&gt;1000 km. Suitable sources must contain significant correlated flux
density (&gt;50-100 mJy) at frequencies around 110-190 MHz on scales of a
few hundred milliarcseconds. If you use this data, cite Jackson et al.
2016 (A&amp;A 595A, 86J). For a description of the catalog format, see
https://www.jb.man.ac.uk/~njj/lbcs_stats.sum.</description><source format="bibcode">2016A&amp;A...595A..86J</source><referenceURL>https://vo.astron.nl/lbcs/lobos/cone/info</referenceURL></content><facility>LOFAR</facility><coverage><waveband>Radio</waveband></coverage><tableset><schema><name>lbcs</name><title>LBCS Calibrator Search</title><description> This service queries the catalog of calibrators from the LOFAR
Long-Baseline Calibrator Survey (LBCS). The LBCS aims to identify
sources suitable for calibrating the highest-resolution observations
made with the International LOFAR Telescope, which include baselines
&gt;1000 km. Suitable sources must contain significant correlated flux
density (&gt;50-100 mJy) at frequencies around 110-190 MHz on scales of a
few hundred milliarcseconds. If you use this data, cite Jackson et al.
2016 (A&amp;A 595A, 86J). For a description of the catalog format, see
https://www.jb.man.ac.uk/~njj/lbcs_stats.sum.</description><table><name>lbcs.main</name><description> This service queries the catalog of calibrators from the LOFAR
Long-Baseline Calibrator Survey (LBCS). The LBCS aims to identify
sources suitable for calibrating the highest-resolution observations
made with the International LOFAR Telescope, which include baselines
&gt;1000 km. Suitable sources must contain significant correlated flux
density (&gt;50-100 mJy) at frequencies around 110-190 MHz on scales of a
few hundred milliarcseconds. If you use this data, cite Jackson et al.
2016 (A&amp;A 595A, 86J). For a description of the catalog format, see
https://www.jb.man.ac.uk/~njj/lbcs_stats.sum.</description><column><name>obsid</name><description>LOFAR Observation ID</description><ucd>meta.id;meta.main</ucd><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType><flag>indexed</flag><flag>primary</flag></column><column><name>raj2000</name><description>Source J2000 Right Ascension, in decimal degrees.</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>indexed</flag></column><column><name>decj2000</name><description>Source J2000 Declination, in decimal degrees.</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>indexed</flag></column><column><name>obsdate</name><description>Observation date.</description><ucd>time.epoch;obs</ucd><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType></column><column><name>obstime</name><description>Observation time.</description><ucd>time.epoch;obs</ucd><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType></column><column><name>baselinequal</name><description>Goodness of the calibrator on the international stations, judged by signal-to-noise ratio of the fringe fit.</description><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType></column><column><name>obsqual</name><description>Quality of the observation, judged by the percentage of source detections on the shorter baselines.</description><dataType xsi:type="vs:VOTableType">short</dataType></column><column><name>baselinequalft</name><description>Goodness of the calibrator on the international stations, judged by signal-to-noise of the Fourier transform of the data.</description><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType></column><column><name>obsflag</name><description>Observation flag.</description><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType></column></table></schema></tableset></ri:Resource>