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<ri:Resource created="2017-04-13T08:27:44Z" 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>GTC transit light curves of WASP-52b</title><shortName>J/A+A/600/L11</shortName><identifier>ivo://CDS.VizieR/J/A+A/600/L11</identifier><altIdentifier>doi:10.26093/cds/vizier.36009011</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Chen G.</name></creator><creator><name>Palle E.</name></creator><creator><name>Nortmann L.</name></creator><creator><name>Murgas F.</name></creator><creator><name>Parviainen H.</name></creator><creator><name>Nowak G.</name></creator><date role="Updated">2017-07-03T14:25:56Z</date><date role="Created">2017-04-13T08:27:44Z</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>multiple-stars</subject><subject>solar-system-planets</subject><subject>spectroscopy</subject><description>We report the first detection of sodium absorption in the atmosphere of the hot Jupiter WASP-52b. We observed one transit of WASP-52b with the low-resolution Optical System for Imaging and low-Intermediate-Resolution Integrated Spectroscopy (OSIRIS) at the 10.4m Gran Telescopio Canarias (GTC). The resulting transmission spectrum, covering the wavelength range from 522nm to 903nm, is flat and featureless, except for the significant narrow absorption signature at the sodium doublet, which can be explained by an atmosphere in solar composition with clouds at 1 mbar. A cloud-free atmosphere is stringently ruled out. By assessing the absorption depths of sodium in various bin widths, we find that temperature increases towards lower atmospheric pressure levels, with a positive temperature gradient of 0.88+/-0.65K/km , possibly indicative of upper atmospheric heating and a temperature inversion.</description><source format="bibcode">2017A&amp;A...600L..11C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/600/L11</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>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/563/A41">J/A+A/563/A41 : WASP-43 OSIRIS transmission spectroscopy (Murgas+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/589/A62">J/A+A/589/A62 : GTC transit light curves of CoRoT-29b (Palle+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/594/A65">J/A+A/594/A65 : GTC transit light curves of HAT-P-32b (Nortmann+, 2016)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/600/L11</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/600/L11</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/600/L11</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/600/L11</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/600/L11</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/600/L11</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><coverage><footprint ivo-id="ivo://ivoa.net/std/moc"/><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/A+A/600/L11/list</name><description>List of spectroscopic light curves</description><column><name>Title</name><description>Title of the file</description><ucd>meta.title;meta.file</ucd><dataType xsi:type="vs:VOTableType" arraysize="76*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. 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