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Journal articles
BLAST: A Far-Infrared Measurement of the History of Star Formation
Enzo Pascale
Peter A. R. Ade
James J. Bock
Edward L. Chapin
Mark J. Devlin
Simon Dye
Steve A. Eales
Matthew Griffin
Joshua O. Gundersen
Mark Halpern
Peter C. Hargrave
David H. Hughes
Jeff Klein
Gaelen Marsden
Philip Mauskopf
Lorenzo Moncelsi
Calvin B. Netterfield
Luca Olmi
G. Patanchon
1
Marie Rex
Douglas Scott
Christopher Semisch
Nicholas Thomas
Matthew D. P. Truch
Carole Tucker
Gregory S. Tucker
Marco P. Viero
Donald V. Wiebe
1
APC - Cosmologie (France)
- APC (UMR_7164) - AstroParticule et Cosmologie (APC - UMR 7164, Université Paris Diderot, 10 rue Alice Domon et Léonie Duquet, case postale 7020, F-75205 Paris Cedex 13 - France)
- Observatoire de Paris (61 Av de l'Observatoire 75014 PARIS - France)
- PSL - Université Paris sciences et lettres (60 rue Mazarine 75006 Paris - France)
- CEA - Commissariat à l'énergie atomique et aux énergies alternatives : DRF/IRFU (Centre de Saclay Centre de Grenoble Centre de Cadarache etc - France)
- UPD7 - Université Paris Diderot - Paris 7 : UMR_7164 (5 rue Thomas-Mann - 75205 Paris cedex 13 - France)
- CNRS - Centre National de la Recherche Scientifique : UMR_7164 (France)
- IN2P3 - Institut National de Physique Nucléaire et de Physique des Particules du CNRS (France)
- Observatoire de Paris (61 Av de l'Observatoire 75014 PARIS - France)
Abstract : We use measurements from the Balloon-borne Large Aperture Sub-millimeter Telescope (BLAST) at wavelengths spanning 250 to 500 microns, combined with data from the Spitzer Infrared telescope and ground-based optical surveys in GOODS-S, to determine the average star formation rate of the galaxies that comprise the cosmic infrared background (CIB) radiation from 70 to 500 microns, at redshifts 0 < z < 3. We find that different redshifts are preferentially probed at different wavelengths within this range, with most of the 70 micron background generated at z < ~1 and the 500 micron background generated at z > ~1. The spectral coverage of BLAST and Spitzer in the region of the peak of the background at ~200 microns allows us to directly estimate the mean physical properties (temperature, bolometric luminosity and mass) of the dust in the galaxies responsible for contributing more than 80% of the CIB. By utilizing available redshift information we directly measure the evolution of the far infrared luminosity density and therefore the optically obscured star formation history up to redshift z ~3.
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Journal articles
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http://hal.in2p3.fr/in2p3-00376814
Contributor : Simone Lantz <>
Submitted on : Monday, April 20, 2009 - 12:14:34 PM
Last modification on : Wednesday, October 21, 2020 - 4:32:14 PM
Contributor : Simone Lantz <>
Submitted on : Monday, April 20, 2009 - 12:14:34 PM
Last modification on : Wednesday, October 21, 2020 - 4:32:14 PM
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Identifiers
- HAL Id : in2p3-00376814, version 1
- ARXIV : 0904.1206
- BIBCODE : 2009ApJ...707.1740P
- DOI : 10.1088/0004-637X/707/2/1740
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IN2P3 | OBSPM | CEA | APC | CNRS | UNIV-PARIS7 | USPC | IRFU-APC | DSM-IRFU | CEA-DRF | UNIV-PARIS | UP-SCIENCES | PSL
Citation
Enzo Pascale, Peter A. R. Ade, James J. Bock, Edward L. Chapin, Mark J. Devlin, et al.. BLAST: A Far-Infrared Measurement of the History of Star Formation. The Astrophysical Journal, American Astronomical Society, 2009, 707, pp.1740-1749. ⟨10.1088/0004-637X/707/2/1740⟩. ⟨in2p3-00376814⟩
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