The COS Legacy Archive Spectroscopy Survey (CLASSY) Treasury Atlas
| dc.contributor.author | Berg, Danielle | |
| dc.contributor.author | James, Bethan L. | |
| dc.contributor.author | King, Teagan | |
| dc.contributor.author | McDonald, Meaghan | |
| dc.contributor.author | Chen, Zuyi | |
| dc.contributor.author | Chisholm, John | |
| dc.contributor.author | Heckman, Timothy | |
| dc.contributor.author | Martin, Crystal L | |
| dc.contributor.author | Stark, Daniel P | |
| dc.contributor.author | Aloisi, Alessandra | |
| dc.contributor.author | Kewley, Lisa | |
| dc.date.accessioned | 2025-04-08T01:21:38Z | |
| dc.date.available | 2025-04-08T01:21:38Z | |
| dc.date.issued | 2022 | |
| dc.date.updated | 2023-12-17T07:16:33Z | |
| dc.description.abstract | Far-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.sponsorship | Funding 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.mimetype | application/pdf | en_AU |
| dc.identifier.issn | 0067-0049 | |
| dc.identifier.uri | https://hdl.handle.net/1885/733747291 | |
| dc.language.iso | en_AU | en_AU |
| dc.provenance | Original 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.publisher | Institute of Physics Publishing | |
| dc.rights | ©2022 The authors | |
| dc.rights.license | Creative Commons Attribution licence | |
| dc.rights.uri | http://creativecommons.org/licenses/by/4.0/ | |
| dc.source | Astrophysical Journal Supplement Series | |
| dc.title | The COS Legacy Archive Spectroscopy Survey (CLASSY) Treasury Atlas | |
| dc.type | Journal article | |
| dcterms.accessRights | Open Access | |
| local.bibliographicCitation.issue | 31 | |
| local.contributor.affiliation | Berg, Danielle, University of Texas at Austin | |
| local.contributor.affiliation | James, Bethan L., Space Telescope Science Institute | |
| local.contributor.affiliation | King, Teagan, Space Telescope Science Institute | |
| local.contributor.affiliation | McDonald, Meaghan, Space Telescope Science Institute | |
| local.contributor.affiliation | Chen, Zuyi, Steward Observatory | |
| local.contributor.affiliation | Chisholm, John, University of Texas Austin | |
| local.contributor.affiliation | Heckman, Timothy, Johns Hopkins University | |
| local.contributor.affiliation | Martin, Crystal L, University of California | |
| local.contributor.affiliation | Stark, Daniel P, University of Arizona | |
| local.contributor.affiliation | Aloisi, Alessandra, Space Telescope Science Institute | |
| local.contributor.affiliation | Kewley, Lisa, College of Science, ANU | |
| local.contributor.authoruid | Kewley, Lisa, u9415124 | |
| local.description.notes | Imported from ARIES | |
| local.identifier.absfor | 510100 - Astronomical sciences | |
| local.identifier.absseo | 280120 - Expanding knowledge in the physical sciences | |
| local.identifier.ariespublication | a383154xPUB40511 | |
| local.identifier.citationvolume | 261 | |
| local.identifier.doi | 10.3847/1538-4365/ac6c03 | |
| local.identifier.scopusID | 2-s2.0-85149567449 | |
| local.publisher.url | https://iopscience.iop.org/ | |
| local.type.status | Published Version | |
| publicationvolume.volumeNumber | 261 |
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