IAC (Spain) This development has been supported by the funding agencies BMVIT (Austria ASI/INAF (Italy), and CICYT/MCYT (Spain) SPIRE has been developed by a consortium of institutes led by Cardiff Univ. (UK) and including: Univ. Lethbridge (Canada); NAOC (China); CEA, LAM (France); IFSI, Univ. Padua (Italy); IAC (Spain); Stockholm Observatory (Sweden), This development has been supported by national funding agencies ,
ASI (Italy); MCINN (Spain); SNSB (Sweden) ,
IAC (Spain) Stockholm Observatory (Sweden) Imperial University of Sussex (UK); and Caltech This development has been supported by national funding agencies: CSA (Canada); NAOC (China), Italy) ,
??? 8 LYMAN-BREAK GALAXIES IN THE ULTRA-DEEP HUDF09 AND WIDE-AREA EARLY RELEASE SCIENCE WFC3/IR OBSERVATIONS, The Astrophysical Journal, vol.737, issue.2, p.90, 2011. ,
DOI : 10.1088/0004-637X/737/2/90
??? 4 STAR-FORMING GALAXIES, The Astrophysical Journal, vol.754, issue.2, p.83, 2012. ,
DOI : 10.1088/0004-637X/754/2/83
= 1, Astronomy and Astrophysics, vol.507, issue.2, p.693, 2009. ,
DOI : 10.1051/0004-6361/200912024
/SPIRE, The Astrophysical Journal, vol.734, issue.1, pp.12-761, 2011. ,
DOI : 10.1088/2041-8205/734/1/L12
URL : https://hal.archives-ouvertes.fr/hal-00662136
Interpreting the Cosmic Infrared Background: Constraints on the Evolution of the Dust???enshrouded Star Formation Rate, The Astrophysical Journal, vol.556, issue.2, p.562, 2001. ,
DOI : 10.1086/321609
Ratio, The Astrophysical Journal, vol.637, issue.1, p.242, 2006. ,
DOI : 10.1086/498296
URL : https://hal.archives-ouvertes.fr/hal-00019593
The star formation rate density and dust attenuation evolution over 12??Gyr with the VVDS surveys, Astronomy & Astrophysics, vol.539, issue.670, pp.31-156, 2007. ,
DOI : 10.1051/0004-6361/201118010
URL : https://hal.archives-ouvertes.fr/hal-01428128
THE ORIGIN OF DUST IN THE EARLY UNIVERSE: PROBING THE STAR FORMATION HISTORY OF GALAXIES BY THEIR DUST CONTENT, The Astrophysical Journal, vol.727, issue.2, p.63, 2011. ,
DOI : 10.1088/0004-637X/727/2/63
: an infrared main sequence for star-forming galaxies, Astronomy & Astrophysics, vol.533, issue.426, pp.119-2166, 2010. ,
DOI : 10.1051/0004-6361/201117239
??? 4, The Astrophysical Journal, vol.735, issue.2, p.34, 2011. ,
DOI : 10.1088/2041-8205/735/2/L34
An Observational Determination of the Bolometric Quasar Luminosity Function, The Astrophysical Journal, vol.654, issue.2, p.731, 2007. ,
DOI : 10.1086/509629
STAR FORMATION IN GALAXIES ALONG THE HUBBLE SEQUENCE, Annual Review of Astronomy and Astrophysics, vol.36, issue.1, p.189, 1998. ,
DOI : 10.1146/annurev.astro.36.1.189
??? 3, The Astrophysical Journal, vol.630, issue.1, p.82, 2005. ,
DOI : 10.1086/431894
CONNECTING THE GAMMA RAY BURST RATE AND THE COSMIC STAR FORMATION HISTORY: IMPLICATIONS FOR REIONIZATION AND GALAXY EVOLUTION, The Astrophysical Journal, vol.744, issue.2, p.95, 2012. ,
DOI : 10.1088/0004-637X/744/2/95
???~ 2.5, Astronomy and Astrophysics, vol.515, issue.763, pp.8-129, 2010. ,
DOI : 10.1051/0004-6361/200912058
The evolution of the ultraviolet and infrared luminosity densities
in the universe at 0???<???z???<???1, Astronomy and Astrophysics, vol.440, issue.2, pp.17-755, 2005. ,
DOI : 10.1051/0004-6361:200500158
??? 0.1, The Astrophysical Journal, vol.742, issue.2, p.96, 2011. ,
DOI : 10.1088/0004-637X/742/2/96