Evolution of the luminosity function, star formation rate, morphology, and size of star-forming galaxies selected at rest-frame 1500 and 2800 Å
- Author
- DAHLEN, Tomas1 2 ; MOBASHER, Bahram2 3 ; DICKINSON, Mark4 ; FERGUSON, Henry C2 ; GIAVALISCO, Mauro2 ; KRETCHMER, Claudia5 ; RAVINDRANATH, Swara6
[1] Department of Physics, Stockholm University, 10961, Stockholm, Sweden
[2] Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, United States
[3] Space Telescope Division of the European Space Agency, ESTEC, Noordwijk, Netherlands
[4] National Optical Astronomy Observatory, P.O. Box 26732, Tucson, AZ 85726, United States
[5] Department of Physics and Astronomy, Johns Hopkins University, 3400 North Charles Street, Baltimore, MD 21218, United States
[6] Inter-University Center for Astronomy and Astrophysics, Post Bag-4, Ganeshkhind, Pune, 411007, India - Source
The Astrophysical journal. 2007, Vol 654, Num 1, pp 172-185, 14 p ; 1 ; ref : 1/2 p
- CODEN
- ASJOAB
- ISSN
- 0004-637X
- Scientific domain
- Astronomy earth cosmic environment
- Publisher
- University of Chicago Press, Chicago, IL
- Publication country
- United States
- Document type
- Article
- Language
- English
- Author keyword
- cosmology: observations galaxies: distances and redshifts galaxies: evolution galaxies: formation galaxies: high-redshift
- Keyword (fr)
- Cosmologie Déplacement vers le rouge Fonction luminosité Formation galaxies Formation stellaire Galaxies Morphologie Taux formation Evolution galaxies
- Keyword (en)
- Cosmology Red shift Luminosity function Galaxy formation Star formation Galaxies Morphology Formation rate Galaxy evolution
- Keyword (es)
- Grado formación Evolución galaxias
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 18442443
Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS
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DOI
10.1086/508854 
https://dx.doi.org/10.1086/508854
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