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<ri:Resource created="2014-08-06T14:49:19Z" 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>300-2500nm flux calibration reference spectra</title><shortName>J/A+A/568/A9</shortName><identifier>ivo://CDS.VizieR/J/A+A/568/A9</identifier><altIdentifier>doi:10.26093/cds/vizier.35680009</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Moehler S.</name></creator><creator><name>Modigliani A.</name></creator><creator><name>Freudling W.</name></creator><creator><name>Giammichele N.</name></creator><creator><name>Gianninas A.,Gonneau A.</name></creator><creator><name>Kausch W.</name></creator><creator><name>Lancon A.</name></creator><creator><name>Noll S.</name></creator><creator><name>Rauch T.</name></creator><creator><name>Vinther J.</name></creator><date role="Updated">2015-01-17T16:42:41Z</date><date role="Created">2014-08-06T14:49:19Z</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>spectrophotometry</subject><subject>standard-stars</subject><subject>white-dwarf-stars</subject><description>While the near-infrared wavelength regime is becoming more and more important for astrophysics there is a marked lack of spectrophotometric standard star data that allow to flux calibrate such data. Furthermore flux calibrating medium to high resolution echelle spectroscopy data is challenging even in the optical wavelength range, because the available flux standard data are often too coarsely sampled. We will provide standard star reference data that allow users to derive response curves from 300nm to 2500nm for spectroscopic data of medium to high resolution, including those taken with echelle spectrographs. In addition we describe a method to correct for moderate telluric absorption without the need of observing telluric standard stars. As reference data for the flux standard we use theoretical spectra derived from stellar model atmospheres. We verify that they provide an appropriate description of the observed standard star spectra by checking for residuals in line cores and line overlap regions in the ratios of observed (X-shooter) spectra to model spectra. The finally selected model spectra are then corrected for remaining mismatches and photometrically calibrated using independent observations. The correction of telluric absorption is performed with the help of telluric model spectra. We provide new, finely sampled reference spectra without telluric absorption for six southern flux standard stars that allow the users to flux calibrate their data from 300nm to 2500nm, and a method to correct for telluric absorption using atmospheric models.</description><source format="bibcode">2014A&amp;A...568A...9M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/568/A9</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>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL 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42760 47957</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/568/A9?format=ascii</footprint><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/A+A/568/A9/std</name><description>Model reference spectra for flux standard stars</description><column><name>lambda</name><description>[300/2500] Wavelength {lambda}</description><unit>nm</unit><ucd>em.wl;meta.main</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>primary</flag></column><column><name>GD71</name><description>Model reference spectrum flux for GD71</description><unit>10mW.m**-2.nm**-1</unit><ucd>meta.ref;phot.flux;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>LTT3218</name><description>Model reference spectrum flux for LTT3218</description><unit>10mW.m**-2.nm**-1</unit><ucd>meta.ref;phot.flux;meta.modelled</ucd><dataType 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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>RAJ2000</name><description>Right Ascension J2000</description><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination J2000</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Teff</name><description>[8081/45250] Effective temperature</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>logg</name><description>[5.8/8.2] Surface gravity</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>SpT</name><description>Spectral type</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">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>