THE PERSISTENCE OF COOL GALACTIC WINDS IN HIGH STELLAR MASS GALAXIES BETWEENz∼ 1.4 AND ∼1
- 30 July 2010
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 719 (2) , 1503-1525
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- The SINFONI Mg ii Program for Line Emitters (SIMPLE): Discovering Starbursts near QSO Sight LinesThe Astrophysical Journal, 2007
- The Mass Assembly History of Field Galaxies: Detection of an Evolving Mass Limit for Star‐Forming GalaxiesThe Astrophysical Journal, 2006
- Galaxies in SDSS and DEEP2: A Quiet Life on the Blue Sequence?The Astrophysical Journal, 2006
- New perspectives on strong z≃ 0.5 Mg ii absorbers: are halo mass and equivalent width anticorrelated?Monthly Notices of the Royal Astronomical Society, 2006
- The Mass Assembly Histories of Galaxies of Various Morphologies in the GOODS FieldsThe Astrophysical Journal, 2005
- Toward an Understanding of the Rapid Decline of the Cosmic Star Formation RateThe Astrophysical Journal, 2005
- A Deep Wide-Field, Optical, and Near-Infrared Catalog of a Large Area around the Hubble Deep Field NorthThe Astronomical Journal, 2004
- The Optical and Near‐Infrared Properties of Galaxies. I. Luminosity and Stellar Mass FunctionsThe Astrophysical Journal Supplement Series, 2003
- A New High-Redshift L[CLC]y[/CLC]α Emitter: Possible Superwind Galaxy at [ITAL][CLC]z[/CLC][/ITAL] = 5.69The Astrophysical Journal, 2002
- High‐Redshift Superwinds as the Source of the Strongest MgiiAbsorbers: A Feasibility AnalysisThe Astrophysical Journal, 2001