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<ri:Resource created="2023-06-29T13:03:44Z" 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>Emergent spectral IR fluxes of 122 hot Jupiters</title><shortName>J/AJ/165/104</shortName><identifier>ivo://CDS.VizieR/J/AJ/165/104</identifier><altIdentifier>doi:10.26093/cds/vizier.51650104</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Deming D.</name></creator><creator><name>Line M.R.</name></creator><creator><name>Knutson H.A.</name></creator><creator><name>Crossfield I.J.M.</name></creator><creator><name>Kempton E.M.-R.,Komacek T.D.</name></creator><creator><name>Wallack N.L.</name></creator><creator><name>Fu G.</name></creator><date role="Updated">2023-11-03T12:04:40Z</date><date role="Created">2023-06-29T13:03:44Z</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>exoplanets</subject><subject>infrared-photometry</subject><subject>effective-temperature</subject><description>We study the emergent spectral fluxes of transiting hot Jupiters, using secondary eclipses from Spitzer. To achieve a large and uniform sample, we have reanalyzed all secondary eclipses for all hot Jupiters observed by Spitzer at 3.6 and/or 4.5{mu}m. Our sample comprises 457 eclipses of 122 planets, including eclipses of 13 planets not previously published. We use these eclipse depths to calculate the spectral fluxes emergent from the exoplanetary atmospheres, and thereby infer the temperatures and spectral properties of hot Jupiters. We find that an abrupt rise in brightness temperature, similar to a phase change, occurs on the dayside atmospheres of the population at an equilibrium temperature between 1714 and 1818K (99% confidence limits). The amplitude of the rise is 291{+/-}49K, and two viable causes are the onset of magnetic drag that inhibits longitudinal heat redistribution, and/or the rapid dissipation of dayside clouds. We also study hot Jupiter spectral properties with respect to metallicity and temperature inversions. Models exhibiting 4.5{mu}m emission from temperature inversions reproduce our fluxes statistically for the hottest planets, but the transition to emission is gradual, not abrupt. The Spitzer fluxes are sensitive to metallicity for planets cooler than ~1200K, and most of the hot Jupiter population falls between model tracks having solar to 30x solar metallicity.</description><source format="bibcode">2023AJ....165..104D</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/165/104</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><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/498/L5">J/A+A/498/L5 : Photometry and spectroscopy of HD 80606b (Moutou+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/526/A130">J/A+A/526/A130 : WASP-34b photometry and radial velocities (Smalley+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/426/739">J/MNRAS/426/739 : Velocities for 7 transiting hot Jupiters (Hellier+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/788/92">J/ApJ/788/92 : Hot Jupiter Kepler-13Ab planets occultation (Shporer+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/444/711">J/MNRAS/444/711 : Photometric distances of exoplanets (Triaud+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/813/47">J/ApJ/813/47 : Model atmospheres of irradiated exoplanets (Molliere+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/465/3693">J/MNRAS/465/3693 : 7 WASP-South transiting exoplanets (Hellier+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/610/A20">J/A+A/610/A20 : HITEP. 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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>Name</name><description>Planet b name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType><flag>primary</flag></column><column><name>Rad</name><description>[0.77/2.06] Planet radius in Jupiter radii</description><unit>(7.1492x10+7m)</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Teq</name><description>[736/3921] Planet equilibrium temperature</description><unit>K</unit><ucd>phys.temperature</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>R*</name><description>[0.593/2.69] Stellar radius</description><unit>solRad</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Teff</name><description>[4145/9600] Stellar effective temperature</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>NObs</name><description>Number of eclipse depths observations (table1)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Flux</name><description>Spitzer fluxes (table2)</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>_RA</name><description>Planet position from SIMBAD (right ascension part)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Planet position from SIMBAD (declination part)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table><table><name>J/AJ/165/104/table2</name><description>Emergent fluxes in the 3.6 and 4.5{mu}m bands and brightness temperatures</description><column><name>Name</name><description>Planet b name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. 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