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<ri:Resource created="2020-07-22T12:51:03Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" 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/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd 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>UVIT and GALEX count rates</title><shortName>J/MNRAS/471/3028</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/471/3028</identifier><altIdentifier>doi:10.26093/cds/vizier.74713028</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Rahna P.T.</name></creator><creator><name>Murthy J.</name></creator><creator><name>Safonova M.</name></creator><creator><name>Sutaria F.</name></creator><creator><name>Gudennavar S.B.,Bubbly S.G.</name></creator><date role="Updated">2024-08-17T20:20:25Z</date><date role="Created">2020-07-22T12:51:03Z</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>standard-stars</subject><subject>ultraviolet-photometry</subject><description>We have studied the performance of the Ultraviolet Imaging Telescope payload on AstroSat and derived a calibration of the far-ultraviolet (FUV) and near-ultraviolet (NUV) instruments on board. We find that the sensitivity of both the FUV and NUV channels is as expected from ground calibrations, with the FUV effective area about 35 per cent and the NUV effective area about the same as that of GALEX. The point spread function of the instrument is on the order of 1.2-1.6''. We have found that pixel-to-pixel variations in the sensitivity are less than 10 per cent with spacecraft motion compensating for most of the flat-field variations. 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Star</name><description>[1/2694] Star identification number, within the detector (FUV or NUV)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>RAJ2000</name><description>Right ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>GALEXCR</name><description>GALEX count rate</description><unit>ct/s</unit><ucd>phot.count;em.UV</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>TexpG</name><description>GALEX exposure time</description><unit>s</unit><ucd>time.duration;obs.exposure</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>UVITCR</name><description>UVIT count rate</description><unit>ct/s</unit><ucd>phot.count;em.UV</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>TexpU</name><description>UVIT exposure time</description><unit>s</unit><ucd>time.duration;obs.exposure</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Filt</name><description>Filter (F1, F2, F3, F5 or F6)</description><ucd>meta.id;instr.filter</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>Det</name><description>Detector (FUV or NUV)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column></table></schema></tableset></ri:Resource>