<?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?>
<ri:Resource created="2016-05-31T12:29:50Z" 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>HST/WFC3 NIR photometry of 2M1207b</title><shortName>J/ApJ/818/176</shortName><identifier>ivo://CDS.VizieR/J/ApJ/818/176</identifier><altIdentifier>doi:10.26093/cds/vizier.18180176</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Zhou Y.</name></creator><creator><name>Apai D.</name></creator><creator><name>Schneider G.H.</name></creator><creator><name>Marley M.S.</name></creator><creator><name>Showman A.P.</name></creator><date role="Updated">2017-06-19T07:58:06Z</date><date role="Created">2016-05-31T12:29:50Z</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>Rotational modulations of brown dwarfs have recently provided powerful constraints on the properties of ultra-cool atmospheres, including longitudinal and vertical cloud structures and cloud evolution. Furthermore, periodic light curves directly probe the rotational periods of ultra-cool objects. We present here, for the first time, time-resolved high-precision photometric measurements of a planetary-mass companion, 2M1207b. We observed the binary system with Hubble Space Telescope/Wide Field Camera 3 in two bands and with two spacecraft roll angles. Using point-spread function-based photometry, we reach a nearly photon-noise limited accuracy for both the primary and the secondary. While the primary is consistent with a flat light curve, the secondary shows modulations that are clearly detected in the combined light curve as well as in different subsets of the data. The amplitudes are 1.36% in the F125W and 0.78% in the F160W filters, respectively. By fitting sine waves to the light curves, we find a consistent period of 10.7_-0.6_^+1.2^hr and similar phases in both bands. The J- and H-band amplitude ratio of 2M1207b is very similar to a field brown dwarf that has identical spectral type but different J-H color. Importantly, our study also measures, for the first time, the rotation period for a directly imaged extra-solar planetary-mass companion.</description><source format="bibcode">2016ApJ...818..176Z</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/818/176</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/ApJ/814/65">J/ApJ/814/65 : Jupiter HST light curves (Karalidi+, 2015)</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/A+A/562/A127">J/A+A/562/A127 : NIR integral field spectra of 15 M-L dwarfs (Bonnefoy+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/208/9">J/ApJS/208/9 : Intrinsic colors &amp; temperatures of PMS stars (Pecaut+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/773/168">J/ApJ/773/168 : Submm fluxes of very low-mass stars and BDs (Mohanty+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/747/35">J/ApJ/747/35 : HST/WFC3 transit observation of GJ1214b (Berta+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/517/A76">J/A+A/517/A76 : Near-IR spectrum of 2M1207b (Patience+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/689/1295">J/ApJ/689/1295 : Lithium test implications for BDs (Kirkpatrick+, 2008)</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/818/176</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/818/176</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/818/176</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/818/176</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/818/176</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/818/176</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/818/176/table1</name><description>HST/WFC3 F125W photometry results</description><column><name>Orbit</name><description>[1/6] Orbit number (1)</description><ucd>meta.id;obs</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><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>PA</name><description>[202/227] Position angle</description><unit>deg</unit><ucd>pos.posAng</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Dither</name><description>[1/4] Dither position (2)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Time</name><description>[0/9] Time from start of the observations</description><unit>h</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Flux</name><description>[62867/78848] Primary flux in electrons/s</description><unit>ct/s</unit><ucd>phot.count</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>NFlux</name><description>[0.98/1.01] Normalized primary flux</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>CFlux</name><description>[180/328] Companion flux in electrons/s</description><unit>ct/s</unit><ucd>phot.count</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>NCFlux</name><description>[0.95/1.05] Normalized companion flux</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/ApJ/818/176/table2</name><description>HST/WFC3 F160W photometry results</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>Orbit</name><description>[1/6] Orbit number (1)</description><ucd>meta.id;obs</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>PA</name><description>[202/227] Position angle</description><unit>deg</unit><ucd>pos.posAng</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Dither</name><description>[1/4] Dither position (2)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Time</name><description>[0/9] Time from start of the observations</description><unit>h</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Flux</name><description>[62867/78848] Primary flux in electrons/s</description><unit>ct/s</unit><ucd>phot.count</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>NFlux</name><description>[0.98/1.01] Normalized primary flux</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>CFlux</name><description>[180/328] Companion flux in electrons/s</description><unit>ct/s</unit><ucd>phot.count</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>NCFlux</name><description>[0.95/1.05] Normalized companion flux</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>