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<ri:Resource created="2012-11-30T15:43:18Z" 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>APOSTLE light curve of GJ 1214b</title><shortName>J/ApJ/731/123</shortName><identifier>ivo://CDS.VizieR/J/ApJ/731/123</identifier><altIdentifier>doi:10.26093/cds/vizier.17310123</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Kundurthy P.</name></creator><creator><name>Agol E.</name></creator><creator><name>Becker A.C.</name></creator><creator><name>Barnes R.</name></creator><creator><name>Williams B.</name></creator><creator><name>Mukadam A.</name></creator><date role="Updated">2017-06-21T08:22:37Z</date><date role="Created">2012-11-30T15:43:18Z</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>solar-system-planets</subject><subject>photometry</subject><subject>multiple-stars</subject><description>We present three transits of GJ 1214b, observed as part of the Apache Point Observatory Survey of Transit Light Curves of Exoplanets (APOSTLE). By applying Markov Chain Monte Carlo techniques to a multi-wavelength data set which included our r-band light curves and previously gathered data of GJ 1214b, we confirm earlier estimates of system parameters. Using spectral energy distribution fitting, mass-luminosity relations, and light curve data, we derived absolute parameters for the star and planet, improving uncertainties by a factor of two for the stellar mass (M_*_=0.153^+0.010^_-0.009_M_{sun}_), stellar radius (R_*_=0.210^+0.005^_-0.004R_{sun}_), planetary radius (R_p_=2.74^+0.06^_-0.05_R_{earth}_), and planetary density ({rho}_p_=1.68+/-0.23g/cm^3^). Transit times derived from our study show no evidence for strong transit timing variations. We also report the detection of two features in our light curves which we believe are evidence for a low-energy stellar flare and a spot-crossing event.</description><source format="bibcode">2011ApJ...731..123K</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/731/123</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</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/ApJ/731/123</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/731/123</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/731/123</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/731/123</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/731/123</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/731/123</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/ApJ/731/123/table6</name><description>APOSTLE lightcurve</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Date</name><description>Date of the observation; UTD (2010/04/21, 2010/06/06 and 2010/07/06)</description><ucd>time.epoch</ucd><flag>nullable</flag></column><column><name>Desc</name><description>Light curve description (Flare Data Only, No Flare, No Spot or Spot Data Only)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="15*">char</dataType></column><column><name>BJD</name><description>[-0.105/0.091] Barycentric Julian Date minus mid transit time</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>NFlux</name><description>[0.97/1.01] Normalized flux ratio</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_NFlux</name><description>Error in NFlux</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>MFlux</name><description>[0.98/1] Model light curve (1)</description><ucd>stat.param;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>