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<ri:Resource created="2022-10-26T12:33:57Z" 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>COS Legacy Archive Sp. Survey (CLASSY) treasury</title><shortName>J/ApJS/261/31</shortName><identifier>ivo://CDS.VizieR/J/ApJS/261/31</identifier><altIdentifier>doi:10.26093/cds/vizier.22610031</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Berg D.A.</name></creator><creator><name>James B.L.</name></creator><creator><name>King T.</name></creator><creator><name>McDonald M.</name></creator><creator><name>Chen Z.</name></creator><creator><name>Chisholm J.,Heckman T.</name></creator><creator><name>Martin C.L.</name></creator><creator><name>Stark D.P.</name></creator><creator><name>Aloisi A.</name></creator><creator><name>Amorin R.O.,Arellano-Cordova K.Z.</name></creator><creator><name>Bayliss M.</name></creator><creator><name>Bordoloi R.</name></creator><creator><name>Brinchmann J.</name></creator><creator><name>Charlot S.,Chevallard J.</name></creator><creator><name>Clark I.</name></creator><creator><name>Erb D.K.</name></creator><creator><name>Feltre A.</name></creator><creator><name>Gronke M.</name></creator><creator><name>Hayes M.</name></creator><creator><name>Henry A.,Hernandez S.</name></creator><creator><name>Jaskot A.</name></creator><creator><name>Jones T.</name></creator><creator><name>Kewley L.J.</name></creator><creator><name>Kumari N.</name></creator><creator><name>Leitherer C.,Llerena M.</name></creator><creator><name>Maseda M.</name></creator><creator><name>Mingozzi M.</name></creator><creator><name>Nanayakkara T.</name></creator><creator><name>Ouchi M.</name></creator><creator><name>Plat A.,Pogge R.W.</name></creator><creator><name>Ravindranath S.</name></creator><creator><name>Rigby J.R.</name></creator><creator><name>Sanders R.</name></creator><creator><name>Scarlata C.,Senchyna P.</name></creator><creator><name>Skillman E.D.</name></creator><creator><name>Steidel C.C.</name></creator><creator><name>Strom A.L.</name></creator><creator><name>Sugahara Y.,Wilkins S.M.</name></creator><creator><name>Wofford A.</name></creator><creator><name>Xu X.</name></creator><creator><name>The CLASSY Team</name></creator><date role="Updated">2022-11-09T06:25:47Z</date><date role="Created">2022-10-26T12:33:57Z</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>spectroscopy</subject><subject>ultraviolet-astronomy</subject><subject>visible-astronomy</subject><subject>galaxies</subject><subject>redshifted</subject><subject>chemical-abundances</subject><subject>interstellar-reddening</subject><description>Far-ultraviolet (FUV; ~1200-2000{AA}) spectra are fundamental to our understanding of star-forming galaxies, providing a unique window on massive stellar populations, chemical evolution, feedback processes, and reionization. The launch of the James Webb Space Telescope will soon usher in a new era, pushing the UV spectroscopic frontier to higher redshifts than ever before; however, its success hinges on a comprehensive understanding of the massive star populations and gas conditions that power the observed UV spectral features. This requires a level of detail that is only possible with a combination of ample wavelength coverage, signal-to-noise, spectral-resolution, and sample diversity that has not yet been achieved by any FUV spectral database. We present the Cosmic Origins Spectrograph Legacy Spectroscopic Survey (CLASSY) treasury and its first high-level science product, the CLASSY atlas. CLASSY builds on the Hubble Space Telescope (HST) archive to construct the first high-quality (S/N_1500{AA}_&gt;~5/resel), high-resolution (R~15000) FUV spectral database of 45 nearby (0.002&lt;z&lt;0.182) star-forming galaxies. The CLASSY atlas, available to the public via the CLASSY website, is the result of optimally extracting and coadding 170 archival+new spectra from 312 orbits of HST observations. The CLASSY sample covers a broad range of properties including stellar mass (6.2&lt;logM_*_(M_{sun}_)&lt;10.1), star formation rate (-2.0&lt;logSFR(M_{sun}_/yr)&lt;+1.6), direct gas-phase metallicity (7.0&lt;12+log(O/H)&lt;8.8), ionization (0.5&lt;O_32_&lt;38.0), reddening (0.02&lt;E(B-V)&lt;0.67), and nebular density (10&lt;n_e_(cm-3)&lt;1120). CLASSY is biased to UV-bright star-forming galaxies, resulting in a sample that is consistent with the z~0 mass-metallicity relationship, but is offset to higher star formation rates by roughly 2dex, similar to z&gt;~2 galaxies. This unique set of properties makes the CLASSY atlas the benchmark training set for star-forming galaxies across cosmic time.</description><source format="bibcode">2022ApJS..261...31B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/261/31</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/B/hst">B/hst : HST Archived Exposures Catalog (STScI, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/311">II/311 : WISE All-Sky Data Release (Cutri+ 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/147">V/147 : The SDSS Photometric Catalogue, Release 12 (Alam+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/349">II/349 : The Pan-STARRS release 1 (PS1) Survey - DR1 (Chambers+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/335">II/335 : Revised catalog of GALEX UV sources (GUVcat_AIS GR6+7) (Bianchi+ 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/154">V/154 : Sloan Digital Sky Surveys (SDSS), Release 16 (DR16) (Ahumada+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/371">II/371 : The Dark Energy Survey (DES): Data Release 2 (Abott+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/178/247">J/ApJS/178/247 : H{alpha} and [NII] survey in local 11 Mpc (Kennicutt+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/706/599">J/ApJ/706/599 : H{alpha} and UV SFR in the local volume (Lee+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/190/233">J/ApJS/190/233 : Spectroscopy &amp; abundances of SINGS galaxies (Moustakas+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/561/A64">J/A+A/561/A64 : Mrk 996 optical spectroscopy (Telles+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/806/16">J/ApJ/806/16 : CHemical Abundances of Spirals. 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The sample and the spectra (Rigby+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/869/123">J/ApJ/869/123 : Keck Lyman continuum sp. survey (KLCS) (Steidel+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/893/96">J/ApJ/893/96 : CHAOS IV: NGC3184 LBT obs. &amp; 3 other gal. abund. 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Position angle of aperture</description><unit>deg</unit><ucd>pos.posAng;instr.fov</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>ImGFWHM</name><description>[0.1/1.42]? GFWHM along spatial axis of acquisition image</description><unit>arcsec</unit><ucd>phys.angSize</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>f_ImGFWHM</name><description>NA = Not applicable</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>SpData</name><description>Spectrum dataset name</description><ucd>meta.id;meta.dataset</ucd><dataType xsi:type="vs:VOTableType" arraysize="9*">char</dataType></column><column><name>Grating</name><description>Spectrum grating</description><ucd>meta.id;instr</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>clambda</name><description>[1105/2339]? Spectrum central wavelength; in Angstrom units</description><unit>1e-10m</unit><ucd>em.wl.central</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>LP</name><description>[1/4]? Spectrum lifetime position</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>f_LP</name><description>NA = Not applicable</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>lambdaSt</name><description>[966.6/1889.3]? Starting rest wavelength (2)</description><unit>1e-10m</unit><ucd>instr.bandwidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>lambdaEnd</name><description>[1221.7/2414.6]? Ending rest wavelength (2)</description><unit>1e-10m</unit><ucd>instr.bandwidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>