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<ri:Resource created="2026-02-23T08:28:44Z" status="active" updated="2026-02-23T07:34:39Z" 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>Keck/NIRES spectrum for CWISE J105512.11+544328.3</title><shortName>J/ApJ/958/94</shortName><identifier>ivo://CDS.VizieR/J/ApJ/958/94</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Robbins G.</name></creator><creator><name>Meisner A.M.</name></creator><creator><name>Schneider A.C.</name></creator><creator><name>Burgasser A.J.,Kirkpatrick J.D.</name></creator><creator><name>Gagne J.</name></creator><creator><name>Hsu C.-C.</name></creator><creator><name>Moranta L.</name></creator><creator><name>Casewell S.,Marocco F.</name></creator><creator><name>Gerasimov R.</name></creator><creator><name>Faherty J.K.</name></creator><creator><name>Kuchner M.J.</name></creator><creator><name>Caselden D.,Cushing M.C.</name></creator><creator><name>Alejandro S.</name></creator><creator><name>The Backyard Worlds: Planet 9 Collaboration,The Backyard Worlds: Cool Neighbors Collaboration</name></creator><date role="Updated">2026-02-23T07:34:39Z</date><date role="Created">2026-02-23T08:28:44Z</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>y-dwarfs</subject><subject>brown-dwarfs</subject><subject>infrared-astronomy</subject><subject>spectroscopy</subject><description>Y dwarfs, the coolest known spectral class of brown dwarfs, overlap in mass and temperature with giant exoplanets, providing unique laboratories for studying low-temperature atmospheres. However, only a fraction of Y dwarf candidates have been spectroscopically confirmed. We present Keck/NIRES near-infrared spectroscopy of the nearby (d~6-8pc) brown dwarf CWISE J105512.11+544328.3. Although its near-infrared spectrum aligns best with the Y0 standard in the J band, no standard matches well across the full YJHK wavelength range. The CWISE J105512.11+544328.3 NH3-H=0.427+/-0.0012 and CH4-J=0.0385+/-0.0007 absorption indices and absolute Spitzer [4.5] magnitude of 15.18+/-0.22 are also indicative of an early-Y dwarf rather than a late-T dwarf. CWISE J105512.11+544328.3 additionally exhibits the bluest Spitzer [3.6]-[4.5] color among all spectroscopically confirmed Y dwarfs. Despite this anomalously blue Spitzer color given its low luminosity, CWISE J105512.11+544328.3 does not show other clear kinematic or spectral indications of low metallicity. Atmospheric model comparisons yield a log(g)&lt;=4.5 and Teff~500+/-150K for this source. We classify CWISE J105512.11+544328.3 as a Y0 (pec) dwarf, adding to the remarkable diversity of the Y-type population. JWST spectroscopy would be crucial to understanding the origin of this Y dwarf's unusual preference for low-gravity models and blue 3-5{mu}m color.</description><source format="bibcode">2023ApJ...958...94R</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/958/94</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/II/328">II/328 : AllWISE Data Release (Cutri+ 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/365">II/365 : The CatWISE2020 catalog (updated version 28-Jan-2021) (Marocco+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/355">I/355 : Gaia DR3 Part 1. Main source (Gaia Collaboration, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/127/2856">J/AJ/127/2856 : Brown dwarfs in the 2MASS Survey (Burgasser+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/637/1067">J/ApJ/637/1067 : Near-IR spectral classification of T dwarfs (Burgasser+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/137/1">J/AJ/137/1 : PMs and astrometry of late-type dwarfs (Faherty+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/190/100">J/ApJS/190/100 : NIR proper motion survey using 2MASS (Kirkpatrick+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/197/19">J/ApJS/197/19 : First brown dwarfs discovered by WISE (Kirkpatrick+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/144/148">J/AJ/144/148 : Infrared phot. of brown dwarf and Hyper-LIRG (Griffith+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/753/156">J/ApJ/753/156 : T/Y brown dwarfs with WISE photometry (Kirkpatrick+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/205/6">J/ApJS/205/6 : T dwarf population revealed by WISE (Mace+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/794/143">J/ApJ/794/143 : New SpeX Observations of M7-L6 Dwarfs (Bardalez+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/810/158">J/ApJ/810/158 : M,L,T dwarfs fundamental param. and SEDs (Filippazzo+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/842/118">J/ApJ/842/118 : Brown dwarfs with spectral type later than T6 (Leggett+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/856/23">J/ApJ/856/23 : BANYAN. 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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>pmRA</name><description>[-1518.7] Proper motion in right ascension direction (pmRA*cosDE) (1)</description><unit>mas/yr</unit><ucd>pos.pm;pos.eq.ra</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_pmRA</name><description>[2.1] pmRA uncertainty</description><unit>mas/yr</unit><ucd>stat.error;pos.pm;pos.eq.ra</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>pmDE</name><description>[-222.7] Proper motion in declination direction (1)</description><unit>mas/yr</unit><ucd>pos.pm;pos.eq.dec</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_pmDE</name><description>[2] pmDE uncertainty</description><unit>mas/yr</unit><ucd>stat.error;pos.pm;pos.eq.dec</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>muTot</name><description>[1534.9] Total proper motion (1)</description><unit>mas/yr</unit><ucd>pos.pm</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_muTot</name><description>[2.9] muTot uncertainty</description><unit>mas/yr</unit><ucd>stat.error;pos.pm</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>plx</name><description>[145] Parallax (1)</description><unit>mas</unit><ucd>pos.parallax.trig</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_plx</name><description>[14.7] Parallax uncertainty</description><unit>mas</unit><ucd>stat.error;pos.parallax</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Vtan</name><description>[50.2] Tangential velocity; this work</description><unit>km/s</unit><ucd>phys.veloc.transverse</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Vtan</name><description>[5.2] Vtan uncertainty</description><unit>km/s</unit><ucd>stat.error;phys.veloc.transverse</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>SpT</name><description>Spectral type; this work</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>e_SpT</name><description>[0.5] SpT uncertainty</description><ucd>stat.error;src.spType</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Teff</name><description>[500] Effective temperature; this work</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>e_Teff</name><description>[150] Teff uncertainty</description><unit>K</unit><ucd>stat.error;phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>l_logg</name><description>[&lt;=] Limit flag on logg</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>logg</name><description>Log of surface gravity; 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