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<ri:Resource created="2021-12-22T17:42:55Z" 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>Gaia 19bld spectroscopic follow-up</title><shortName>J/A+A/657/A17</shortName><identifier>ivo://CDS.VizieR/J/A+A/657/A17</identifier><altIdentifier>doi:10.26093/cds/vizier.36570017</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Bachelet E.</name></creator><creator><name>Zielinski P.</name></creator><creator><name>Gromadzki M.</name></creator><creator><name>Gezer I.</name></creator><creator><name>Rybicki K.,Kruszynska K.</name></creator><creator><name>Ihanec N.</name></creator><creator><name>Wyrzykowski L.</name></creator><creator><name>Street R.A.</name></creator><creator><name>Tsapras Y.,Hundertmark M.</name></creator><creator><name>Cassan A.</name></creator><creator><name>Harbeck D.</name></creator><creator><name>Rabus M.</name></creator><date role="Updated">2022-03-21T09:21:49Z</date><date role="Created">2021-12-22T17:42:55Z</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>gravitational-lensing</subject><subject>spectroscopy</subject><description>As the event displayed an increased brightness, spectroscopic follow-up observations were immediately scheduled. Low-resolution spectra (R~500) were obtained using the FLOYDS spectrograph, which is mounted on the Las Cumbres Observatory (LCO) 2-m telescope at Siding Spring Observatory In addition,we used the X-shooter instrument mounted on the ESO Very Large Telescope (VLT) which is a multi-wavelength, medium-resolution spectrograph consisted of three spectroscopic arms allowing for simultaneous observations at three wavelength ranges: UVB (300-559.5nm), VIS (559.5-1024nm), and NIR (1024-2480nm). 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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>Inst</name><description>Instrument</description><ucd>meta.id;instr</ucd><dataType xsi:type="vs:VOTableType" arraysize="12*">char</dataType></column><column><name>Obs.date</name><description>Observaton date</description><ucd>time.epoch</ucd><flag>nullable</flag></column><column><name>FileName</name><description>Name of the table with spectrum in subdirectory sp</description><ucd>meta.id;meta.table</ucd><dataType xsi:type="vs:VOTableType" arraysize="25*">char</dataType></column><column><name>sp</name><description>Show the spectrum</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column></table></schema></tableset></ri:Resource>