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The COS Legacy Archive Spectroscopy Survey (CLASSY) Treasury Atlas

dc.contributor.authorBerg, Danielle
dc.contributor.authorJames, Bethan L.
dc.contributor.authorKing, Teagan
dc.contributor.authorMcDonald, Meaghan
dc.contributor.authorChen, Zuyi
dc.contributor.authorChisholm, John
dc.contributor.authorHeckman, Timothy
dc.contributor.authorMartin, Crystal L
dc.contributor.authorStark, Daniel P
dc.contributor.authorAloisi, Alessandra
dc.contributor.authorKewley, Lisa
dc.date.accessioned2025-04-08T01:21:38Z
dc.date.available2025-04-08T01:21:38Z
dc.date.issued2022
dc.date.updated2023-12-17T07:16:33Z
dc.description.abstractFar-ultraviolet (FUV; ∼1200-2000 Å)) 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/N1500 Å  5/resel)), high-resolution (R ∼ 15,000) FUV spectral database of 45 nearby (0.002 < z < 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 < log M ⋆(M ⊙) < 10.1), star formation rate (−2.0 < log SFR (M ⊙ yr−1) < +1.6), direct gas-phase metallicity (7.0 < 12+log(O/H) < 8.8), ionization (0.5 < O32 < 38.0), reddening (0.02 < E(B − V) < 0.67), and nebular density (10 < n e (cm−3) < 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 2 dex, similar to z ≳ 2 galaxies. This unique set of properties makes the CLASSY atlas the benchmark training set for star-forming galaxies across cosmic time.
dc.description.sponsorshipFunding for SDSS-III has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, and the U.S. Department of Energy Office of Science. The SDSS-III website is http://www.sdss3.org/.
dc.format.mimetypeapplication/pdfen_AU
dc.identifier.issn0067-0049
dc.identifier.urihttps://hdl.handle.net/1885/733747291
dc.language.isoen_AUen_AU
dc.provenanceOriginal content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of thework, journal citation and DOI.
dc.publisherInstitute of Physics Publishing
dc.rights©2022 The authors
dc.rights.licenseCreative Commons Attribution licence
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/
dc.sourceAstrophysical Journal Supplement Series
dc.titleThe COS Legacy Archive Spectroscopy Survey (CLASSY) Treasury Atlas
dc.typeJournal article
dcterms.accessRightsOpen Access
local.bibliographicCitation.issue31
local.contributor.affiliationBerg, Danielle, University of Texas at Austin
local.contributor.affiliationJames, Bethan L., Space Telescope Science Institute
local.contributor.affiliationKing, Teagan, Space Telescope Science Institute
local.contributor.affiliationMcDonald, Meaghan, Space Telescope Science Institute
local.contributor.affiliationChen, Zuyi, Steward Observatory
local.contributor.affiliationChisholm, John, University of Texas Austin
local.contributor.affiliationHeckman, Timothy, Johns Hopkins University
local.contributor.affiliationMartin, Crystal L, University of California
local.contributor.affiliationStark, Daniel P, University of Arizona
local.contributor.affiliationAloisi, Alessandra, Space Telescope Science Institute
local.contributor.affiliationKewley, Lisa, College of Science, ANU
local.contributor.authoruidKewley, Lisa, u9415124
local.description.notesImported from ARIES
local.identifier.absfor510100 - Astronomical sciences
local.identifier.absseo280120 - Expanding knowledge in the physical sciences
local.identifier.ariespublicationa383154xPUB40511
local.identifier.citationvolume261
local.identifier.doi10.3847/1538-4365/ac6c03
local.identifier.scopusID2-s2.0-85149567449
local.publisher.urlhttps://iopscience.iop.org/
local.type.statusPublished Version
publicationvolume.volumeNumber261

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