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<ri:Resource created="2014-04-08T07:15:05Z" 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>Light curves of HD 149026b in 3.6-16um</title><shortName>J/ApJ/754/136</shortName><identifier>ivo://CDS.VizieR/J/ApJ/754/136</identifier><altIdentifier>doi:10.26093/cds/vizier.17540136</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Stevenson K.B.</name></creator><creator><name>Harrington J.</name></creator><creator><name>Fortney J.J.</name></creator><creator><name>Loredo T.J.</name></creator><creator><name>Hardy R.A.,Nymeyer S.</name></creator><creator><name>Bowman W.C.</name></creator><creator><name>Cubillos P.</name></creator><creator><name>Bowman M.O.</name></creator><creator><name>Hardin M.</name></creator><date role="Updated">2014-04-20T18:01:01Z</date><date role="Created">2014-04-08T07:15:05Z</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>infrared-photometry</subject><subject>solar-system-planets</subject><description>The dayside of HD 149026b is near the edge of detectability by the Spitzer Space Telescope. We report on 11 secondary-eclipse events at 3.6, 4.5, 3x5.8, 4x8.0, and 2x16{mu}m plus three primary-transit events at 8.0{mu}m. The eclipse depths from jointly fit models at each wavelength are 0.040%+/-0.003% at 3.6{mu}m, 0.034%+/-0.006% at 4.5{mu}m, 0.044%+/-0.010% at 5.8{mu}m, 0.052%+/-0.006% at 8.0{mu}m, and 0.085%+/-0.032% at 16{mu}m. Multiple observations at the longer wavelengths improved eclipse-depth signal-to-noise ratios by up to a factor of two and improved estimates of the planet-to-star radius ratio (R_p_/R_{sstarf}_=0.0518+/-0.0006). We also identify no significant deviations from a circular orbit and, using this model, report an improved period of 2.8758916+/-0.0000014 days. Chemical-equilibrium models find no indication of a temperature inversion in the dayside atmosphere of HD 149026b. Our best-fit model favors large amounts of CO and CO_2_, moderate heat redistribution (f=0.5), and a strongly enhanced metallicity. These analyses use BiLinearly-Interpolated Subpixel Sensitivity (BLISS) mapping, a new technique to model two position-dependent systematics (intrapixel variability and pixelation) by mapping the pixel surface at high resolution. BLISS mapping outperforms previous methods in both speed and goodness of fit. We also present an orthogonalization technique for linearly correlated parameters that accelerates the convergence of Markov chains that employ the Metropolis random walk sampler.</description><source format="bibcode">2012ApJ...754..136S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/754/136</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/552/A119">J/A+A/552/A119 : Planet-star and moon-planet interaction (Saur+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/527/A140">J/A+A/527/A140 : Mass limits on substellar companions (Reffert+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/414/1278">J/MNRAS/414/1278 : Eccentricities of transiting planets (Pont+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/411/L46">J/MNRAS/411/L46 : Exoplanet magnetic fields (Vidotto+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/141/11">J/AJ/141/11 : Spitzer obs. of planet-host stars (Dodson-Robinson+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/733/68">J/ApJ/733/68 : Exoplanet masses derived from RVs (Brown+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/716/1336">J/ApJ/716/1336 : Stability analysis of single-planet (Kopparapu+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/705/1226">J/ApJ/705/1226 : Planet-bearing stars in Spitzer (Bryden+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/700/L73">J/ApJ/700/L73 : Photospheric fluxes at 24 and 70{mu}m (Kospal+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/692/L9">J/ApJ/692/L9 : Tidal evolution of transiting exoplanets (Levrard+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/675/1531">J/ApJ/675/1531 : Transits of super-Neptune HD 149026b (Winn+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/666/475">J/ApJ/666/475 : Extrasolar planet taxonomy (Marchi+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/649/1010">J/ApJ/649/1010 : Habitability of known exoplanetary systems (Jones+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/646/505">J/ApJ/646/505 : Catalog of nearby exoplanets (Butler+, 2006)</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/754/136</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/754/136</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/754/136</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/754/136</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/754/136</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/754/136</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>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/754/136/table1</name><description>Observation information</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>Label</name><description>Observation label (HD149b[p/s]NN) (1)</description><ucd>meta.id;obs</ucd><dataType xsi:type="vs:VOTableType" arraysize="9*">char</dataType></column><column><name>Date</name><description>Observation date</description><ucd>time.epoch;obs</ucd><flag>nullable</flag></column><column><name>Dur</name><description>[330/499] Duration</description><unit>min</unit><ucd>time.duration</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Exp</name><description>[0.4/14] Frame exposure time</description><unit>s</unit><ucd>pos.frame;obs.field;obs.exposure</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Nfr</name><description>[1050/70000] Total number of frames</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Pipeline</name><description>Spitzer pipeline ("S18.7.0" or "S18.18.0")</description><ucd>meta.software</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>lambda</name><description>[3.6/16] Observation wavelength</description><unit>um</unit><ucd>em.wl;obs</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Ref</name><description>Previous publications (2)</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column><column><name>MJD</name><description>MJD date of observation at start (JD-2400000.5) (3)</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>LC</name><description>Spitzer light curves</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>fits</name><description>Download the FITS table</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>FileName</name><description>Name of FITS file in subdirectory fits (3)</description><ucd>meta.id;meta.fits</ucd><dataType xsi:type="vs:VOTableType" arraysize="60*">char</dataType></column></table></schema></tableset></ri:Resource>