Journal article icon

Journal article

The COS Legacy Archive Spectroscopy Survey (CLASSY) Treasury Atlas*

Abstract:
Far-ultraviolet (FUV; ~1200-2000 angstroms) 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 JWST 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 COS Legacy Spectroscopic SurveY (CLASSY) treasury and its first high level science product, the CLASSY atlas. CLASSY builds on the HST archive to construct the first high-quality (S/N_1500 >~ 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 < logM_star(M_sol) < 10.1), star formation rate (-2.0 < log SFR (M_sol/yr) < +1.6), direct gas-phase metallicity (7.0 < 12+log(O/H) < 8.8), ionization (0.5 < O_32 < 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 z~0 mass-metallicity relationship, but is offset to higher SFRs 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.Comment: Accepted for publication in Ap
Publication status:
Published
Peer review status:
Peer reviewed

Actions

Access Document

Files:
Publisher copy:
10.3847/1538-4365/ac6c03
Publication website:
https://hal-insu.archives-ouvertes.fr/insu-03748234/file/Berg_2022_ApJS_261_31.pdf

Authors

More by this author
Role:
Author
ORCID:
0000-0002-4153-053X
More by this author
Role:
Author
ORCID:
0000-0003-4372-2006
More by this author
Role:
Author
ORCID:
0000-0003-0834-4150
More by this author
Role:
Author
ORCID:
0000-0003-0557-3433
More by this author
Role:
Author
ORCID:
0000-0002-2178-5471


More from this funder
Funder identifier:
10.13039/100013757
Grant:
HST-GO-15840
More from this funder
Funder identifier:
https://ror.org/021nxhr62
Grant:
AST-1108693


Publisher:
American Astronomical Society
Journal:
The Astrophysical Journal: Supplement Series More from this journal
Volume:
261
Issue:
2
Pages:
31-31
Publication date:
2022-07-27
DOI:
EISSN:
1538-4365
ISSN:
0067-0049


Language:
English
Keywords:
Pubs id:
1333739
Local pid:
pubs:1333739
Source identifiers:
W4226484856
Deposit date:
2026-05-05
ARK identifier:
This ORA record was generated from metadata provided by an external service. It has not been edited by the ORA Team.

Terms of use


Views and Downloads






If you are the owner of this record, you can report an update to it here: Report update to this record

TO TOP