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<ri:Resource created="2023-09-05T17:05:00Z" 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>Beyond the local volume. I. HST ultracool dwarfs</title><shortName>J/ApJ/924/114</shortName><identifier>ivo://CDS.VizieR/J/ApJ/924/114</identifier><altIdentifier>doi:10.26093/cds/vizier.19240114</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Aganze C.</name></creator><creator><name>Burgasser A.J.</name></creator><creator><name>Malkan M.</name></creator><creator><name>Theissen C.A.</name></creator><creator><name>Tejada Arevalo R.A.,Hsu C.-C.</name></creator><creator><name>Bardalez Gagliuffi D.C.</name></creator><creator><name>Ryan R.E.</name></creator><creator><name>Holwerda B.</name></creator><date role="Updated">2023-11-09T13:05:00Z</date><date role="Created">2023-09-05T17:05:00Z</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>hst-photometry</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><subject>stellar-spectral-types</subject><subject>stellar-distance</subject><subject>l-dwarfs</subject><subject>m-stars</subject><subject>brown-dwarfs</subject><subject>infrared-sources</subject><subject>surveys</subject><description>Ultracool dwarf stars and brown dwarfs provide a unique probe of large-scale Galactic structure and evolution; however, until recently spectroscopic samples of sufficient size, depth, and fidelity have been unavailable. Here, we present the identification of 164 M7-T9 ultracool dwarfs in 0.6deg^2^ of deep, low-resolution, near-infrared spectroscopic data obtained with the Hubble Space Telescope (HST) Wide Field Camera 3 (WFC3) instrument as part of the WFC3 Infrared Spectroscopic Parallel Survey and the 3D-HST survey. We describe the methodology by which we isolate ultracool dwarf candidates from over 200000 spectra, and show that selection by machine-learning classification is superior to spectral index-based methods in terms of completeness and contamination. We use the spectra to accurately determine classifications and spectrophotometric distances, the latter reaching to ~2kpc for L dwarfs and ~400pc for T dwarfs.</description><source format="bibcode">2022ApJ...924..114A</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/924/114</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/II/246">II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/261">II/261 : GOODS initial results (Giavalisco+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/284">II/284 : COSMOS Multi-Wavelength Photometry Catalog (Capak+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/319">II/319 : UKIDSS-DR9 LAS, GCS and DXS Surveys (Lawrence+ 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/126/1526">J/AJ/126/1526 : IR photometry of ultracool dwarfs (Bouy+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/358/13">J/MNRAS/358/13 : Faint dwarfs in NGC 2547 (Jeffries+, 2005)</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/133/439">J/AJ/133/439 : Luminosity function of M7-L8 ultracool dwarfs (Cruz+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/676/1281">J/ApJ/676/1281 : L and T dwarfs in 2MASS/SDSS (Metchev+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/695/1591">J/ApJ/695/1591 : Spectrophotometry in PEARS fields (Pirzkal+, 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/A+A/522/A112">J/A+A/522/A112 : i'z' phot. of L5 and later dwarf candidates (Reyle+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/414/2602">J/MNRAS/414/2602 : Automated classification of HIP variables (Dubath+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/201/19">J/ApJS/201/19 : Hawaii Infrared Parallax Program. 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