- Abstract:
-
We measure a relation between the depth of four prominent rest-UV absorption complexes and metallicity for local galaxies and verify it up to z ∼ 3. We then apply this relation to a sample of 224 galaxies at 3.5 < z < 6.0 (zñ = 4.8) in the Cosmic Evolution Survey (COSMOS), for which unique UV spectra from the Deep Imaging Multi-object Spectrograph (DEIMOS) and accurate stellar masses from the Spitzer Large Area Survey with Hyper- Suprime-Cam (SPLASH) are available. The average galaxy po...
Expand abstract - Publication status:
- Published
- Peer review status:
- Peer reviewed
- Version:
- Publisher's Version
- Files:
-
-
(pdf, 2.0mb)
-
- Publisher copy:
- 10.3847/0004-637X/822/1/29
-
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- Publisher:
- American Astronomical Society Publisher's website
- Journal:
- Astrophysical Journal Journal website
- Volume:
- 822
- Issue:
- 1
- Pages:
- Article: 29
- Publication date:
- 2016-05-02
- Acceptance date:
- 2016-02-13
- DOI:
- EISSN:
-
1538-4357
- ISSN:
-
0004-637X
- Pubs id:
-
pubs:658473
- URN:
-
uri:16e8b5e1-6592-48f2-a901-5ea1054a2bd0
- UUID:
-
uuid:16e8b5e1-6592-48f2-a901-5ea1054a2bd0
- Local pid:
- pubs:658473
- Keywords:
- Copyright holder:
- American Astronomical Society
- Copyright date:
- 2016
- Notes:
- © 2016. The American Astronomical Society. All rights reserved.
Journal article
Rest-UV absorption lines as metallicity estimator: the metal content of star-forming galaxies at Z ∼ 5
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