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<ri:Resource created="2024-12-04T13:01:34Z" 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>An updated distance-calibrated SED of Gl 229B</title><shortName>J/ApJ/940/164</shortName><identifier>ivo://CDS.VizieR/J/ApJ/940/164</identifier><altIdentifier>doi:10.26093/cds/vizier.19400164</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Calamari E.</name></creator><creator><name>Faherty J.K.</name></creator><creator><name>Burningham B.</name></creator><creator><name>Gonzales E.,Bardalez-Gagliuffi D.</name></creator><creator><name>Vos J.M.</name></creator><creator><name>Gemma M.</name></creator><creator><name>Whiteford N.</name></creator><creator><name>Gaarn J.</name></creator><date role="Updated">2025-02-24T20:13:33Z</date><date role="Created">2024-12-04T13:01:34Z</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>brown-dwarfs</subject><subject>multiple-stars</subject><subject>t-dwarfs</subject><subject>spectral-energy-distribution</subject><subject>infrared-astronomy</subject><subject>spectroscopy</subject><subject>visible-astronomy</subject><subject>astronomical-models</subject><description>We present results from an atmospheric retrieval analysis of Gl 229B using the Brewster retrieval code. We find the best fit model to be cloud-free, consistent with the T dwarf retrieval work of Line+ 2015ApJ...807..183L &amp; 2017ApJ...848...83L; Zalesky+ 2022ApJ...936...44Z and Gonzales+ 2020ApJ...905...46G. Fundamental parameters (mass, radius, log(L_Bol_/L_Sun_), log(g)) determined from our model agree within 1{sigma} to SED-derived values, except for Teff where our retrieved Teff is approximately 100K cooler than the evolutionary model-based SED value. We find a retrieved mass of 50_-9_^+12^M_Jup_, however, we also find that the observables of Gl229B can be explained by a cloud-free model with a prior on mass at the dynamical value, 70M_Jup_. We are able to constrain abundances for H_2_O, CO, CH_4_, NH_3_, Na and K and find a supersolar C/O ratio as compared to its primary, Gl 229A. We report an overall subsolar metallicity due to atmospheric oxygen depletion, but find a solar [C/H], which matches that of the primary. We find that this work contributes to a growing trend in retrieval-based studies, particularly for brown dwarfs, toward supersolar C/O ratios and discuss the implications of this result on formation mechanisms and internal physical processes, as well as model biases.</description><source format="bibcode">2022ApJ...940..164C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/940/164</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/327/1039">J/A+A/327/1039 : Structure and evolution of low-mass stars (Chabrier+ 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/ARA+A/43.195">J/other/ARA+A/43.195 : L and T dwarf stars (Kirkpatrick, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/637/1067">J/ApJ/637/1067 : NIR spectral classification of T dwarfs (Burgasser+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/135/785">J/AJ/135/785 : SDSS-DR5 low-mass star spectroscopic sample (West+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/510/A99">J/A+A/510/A99 : Epsilon Indi Ba and Bb IR spectra (King+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/433/457">J/MNRAS/433/457 : 76 T dwarfs from the UKIDSS LAS (Burningham+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/214/25">J/ApJS/214/25 : Rosseland &amp; Planck gaseous mean opacities (Freedman+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/791/54">J/ApJ/791/54 : Nearby M Dwarfs parameters (Gaidos+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/564/A55">J/A+A/564/A55 : 1.1-2.4um spectra of 7 young M &amp; L dwarfs (Manjavacas+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/216/7">J/ApJS/216/7 : Planets Around Low-Mass Stars (PALMS). 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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>lambda</name><description>[0.6/5.1] Wavelength (1)</description><unit>um</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Flux</name><description>[4.6e-21/4.4e-16] Flux; erg/s/cm^2^/{AA} (2)</description><unit>cW.m**-2.nm**-1</unit><ucd>phot.flux</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_Flux</name><description>[2.3e-22/2.2e-17] Uncertainty in Flux</description><unit>cW.m**-2.nm**-1</unit><ucd>stat.error;phot.flux</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table><table><name>J/ApJ/940/164/fig3</name><description>The temperature-pressure profile</description><column><name>logP</name><description>[-4/2.3] log pressure</description><unit>bar</unit><ucd>phys.pressure</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Temp</name><description>[248/2050] Temperature</description><unit>K</unit><ucd>phys.temperature</ucd><dataType xsi:type="vs:VOTableType">double</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></table><table><name>J/ApJ/940/164/fig4</name><description>The median and maximum likelihood retrieved spectra</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>Model</name><description>Model type (1)</description><ucd>meta.id;stat.fit</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>lambda</name><description>[1.0005/5.005] Wavelength</description><unit>um</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Flux</name><description>[4.17e-18/4.1e-15] Flux</description><unit>W.m**-2.um**-1</unit><ucd>phot.flux;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_Flux</name><description>? Lower uncertainty in Flux (2)</description><unit>W.m**-2.um**-1</unit><ucd>stat.error;phot.flux;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>E_Flux</name><description>? Upper uncertainty in Flux (2)</description><unit>W.m**-2.um**-1</unit><ucd>stat.error;phot.flux;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>