KECK SPECTROSCOPY OF 3 < z < 7 FAINT LYMAN BREAK GALAXIES: THE IMPORTANCE OF NEBULAR EMISSION IN UNDERSTANDING THE SPECIFIC STAR FORMATION RATE AND STELLAR MASS DENSITY (2013)
Attributed to:
Astronomy and Astrophysics at Edinburgh
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1088/0004-637x/763/2/129
Publication URI: http://dx.doi.org/10.1088/0004-637x/763/2/129
Type: Journal Article/Review
Parent Publication: The Astrophysical Journal
Issue: 2
ISSN: 0004-637X