UV CONTINUUM SLOPE AND DUST OBSCURATION FROM z ∼ 6 TO z ∼ 2: THE STAR FORMATION RATE DENSITY AT HIGH REDSHIFT
- Author
- BOUWENS, R. J1 2 ; ILLINGWORTH, G. D1 ; FRANX, M2 ; CHARY, R.-R3 ; MEURER, G. R4 ; CONSELICE, C. J5 ; FORD, H4 ; GIAVALISCO, M6 ; VAN DOKKUM, P7
[1] Astronomy Department, University of California, Santa Cruz, CA 95064, United States
[2] Leiden Observatory, University of Leiden, Postbus 9513, 2300 RA Leiden, Netherlands
[3] Divison of Physics, Mathematics, and Astronomy, California Institute of Technology, Pasadena, CA 91125, United States
[4] Department of Physics and Astronomy, Johns Hopkins University, 3400 North Charles Street, Baltimore, MD 21218, United States
[5] University of Nottingham, School of Physics & Astronomy, Nottinghm NG7 2RD, United Kingdom
[6] Department of Astronomy, University of Massachusetts, Amherst, MA, United States
[7] Department of Astronomy, Yale University, New Haven, CT, United States - Source
The Astrophysical journal. 2009, Vol 705, Num 1, pp 936-961, 26 p ; 1 ; ref : 1 p.1/2
- CODEN
- ASJOAB
- ISSN
- 0004-637X
- Scientific domain
- Astronomy earth cosmic environment
- Publisher
- IOP, Bristol
- Publication country
- United Kingdom
- Document type
- Article
- Language
- English
- Author keyword
- galaxies: evolution galaxies: high-redshift
- Keyword (fr)
- Continuum Densité élevée Déplacement vers le rouge Evolution galaxies Formation stellaire Galaxies Taux formation
- Keyword (en)
- Continuum High density Red shift Galaxy evolution Star formation Galaxies Formation rate
- Keyword (es)
- Continuo Densidad elevada Evolución galaxias Grado formación
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 22162847
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
10.1088/0004-637X/705/1/936 
https://dx.doi.org/10.1088/0004-637X/705/1/936
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