We use medium-resolution Keck/Echellette Spectrograph and Imager spectroscopy of bright quasars to study cool gas traced by Ca
We use a sample of 27 gamma-ray bursts (GRBs) at redshift
- NSF-PAR ID:
- 10362712
- Publisher / Repository:
- DOI PREFIX: 10.3847
- Date Published:
- Journal Name:
- The Astrophysical Journal
- Volume:
- 926
- Issue:
- 1
- ISSN:
- 0004-637X
- Format(s):
- Medium: X Size: Article No. 63
- Size(s):
- ["Article No. 63"]
- Sponsoring Org:
- National Science Foundation
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