GOODS-Herschel: dust attenuation properties of UV selected high redshift galaxies
- Author
- BUAT, V1 ; NOLL, S2 ; REDDY, N11 ; MURPHY, E. J12 ; BURGARELLA, D1 ; GIOVANNOLI, E1 3 ; CHARMANDARIS, V4 5 6 ; PANNELLA, M7 ; HWANG, H. S8 ; ELBAZ, D7 ; DICKINSON, M9 ; MAGDIS, G10
[1] Aix-Marseille Université, CNRS - LAM (Laboratoire d'Astrophysique de Marseille) UMR 7326, 13388 Marseille, France
[2] Institut für Astro- und Teilchenphysik, Universitat Innsbruck, Technikerstr. 25/8, 6020 Innsbruck, Austria
[3] University of the Western Cape, Private Bag X17, 7535 Bellville, Cape Town, South Africa
[4] University of Crete, Department of Physics and Institute of Theoretical & Computational Physics, 71003 Heraklion, Greece
[5] IESL/Foundation for Research & Technology-Hellas, 71110 Heraklion, Greece
[6] Observatoire de Paris, LERMA (CNRS: UMR 8112), 61 Av. de l'Observatoire, 75014 Paris, France
[7] Laboratoire AIM-Paris-Saclay, CEA/DSM/Irfu - CNRS - Universite Paris Diderot, CE-Saclay, 91191 Gif-sur-Yvette, France
[8] Smithsonian Astrophysical Observatory, 60 Garden St, Cambridge, MA 02138, United States
[9] National Optical Astronomy Observatory, 950 North Cherry Avenue, Tucson, AZ 85719, United States
[10] Department of Physics, University of Oxford, Keble Road, Oxford, OX1 3RH, United Kingdom
[11] Department of Physics and Astronomy, University of California, Riverside, 900 University Avenue, Riverside, 92521 California, United States
[12] Spitzer Science Center, California Institute of Technology, Pasadena, CA, 91125, United States - Source
Astronomy and astrophysics (Berlin. Print). 2012, Vol 545 ; A141.1-A141.15 ; 2 ; ref : 1/2 p
- CODEN
- AAEJAF
- ISSN
- 0004-6361
- Scientific domain
- Astronomy earth cosmic environment
- Publisher
- EDP Sciences, Les Ulis
- Publication country
- France
- Document type
- Article
- Language
- English
- Author keyword
- dust, extinction galaxies: ISM galaxies: high-redshift galaxies: starburst ultraviolet: galaxies
- Keyword (fr)
- Age Atténuation Continuum Courbe extinction Densité spectrale énergie Déplacement vers le rouge Formation stellaire Galaxies à flambée Grand Nuage Magellan Luminosité Masse stellaire Paramètre physique Population stellaire Propriété physique Taux formation
- Keyword (en)
- Age Attenuation Continuum Extinction curve Spectral energy distribution Red shift Star formation Starburst galaxies Large Magellanic Cloud Luminosity Stellar mass Physical parameter Stellar population Physical properties Formation rate
- Keyword (es)
- Edad Continuo Curva extinción Densidad espectral energía Galaxias llamarada estelar Parámetro físico Población estelar Grado formación
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 26597913
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
10.1051/0004-6361/201219405 
https://dx.doi.org/10.1051/0004-6361/201219405
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