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<ri:Resource created="2012-03-02T07:56:18Z" 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>CRIRES-POP: high resolution IR spectra library</title><shortName>J/A+A/539/A109</shortName><identifier>ivo://CDS.VizieR/J/A+A/539/A109</identifier><altIdentifier>doi:10.26093/cds/vizier.35390109</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Lebzelter T.</name></creator><creator><name>Seifahrt A.</name></creator><creator><name>Uttenthaler S.</name></creator><creator><name>Ramsay S.</name></creator><creator><name>Hartman H.,Nieva M.F.</name></creator><creator><name>Pryzibilla N.</name></creator><creator><name>Smette A.</name></creator><creator><name>Wahlgren G.M.</name></creator><creator><name>Wolff B.,Hussain G.A.J.</name></creator><creator><name>Kaeufl H.U.</name></creator><creator><name>Seemann U.</name></creator><date role="Updated">2018-01-02T13:42:39Z</date><date role="Created">2012-03-02T07:56:18Z</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>infrared-astronomy</subject><subject>spectroscopy</subject><description>New instrumental capabilities and the wealth of astrophysical information extractable from the near-infrared wavelength region have led to a growing interest in the field of high resolution spectroscopy at 1-5m. We aim to provide a library of observed high-resolution and high signal-to-noise-ratio near-infrared spectra of stars of various types throughout the Hertzsprung-Russell diagram. 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