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 (Q68982982)
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scientific article published in January 2013
- 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
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English | 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 |
scientific article published in January 2013 |
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