GOODS–<i>Herschel</i>: an infrared main sequence for star-forming galaxies

Elbaz, D.; Dickinson, Mark; Seong Hwang, Ho; Díaz-Santos, T.; Magdis, G.; Magnelli, B.; Le Borgne, D.; Galliano, F.; Pannella, M.; Chanial, P.; Armus, L.; Charmandaris, V.; Daddi, E.; Aussel, H.; Popesso, P.; S. Kartaltepe, Jeyhan; Altieri, B.; Valtchanov, I.; Coia, D.; Dannerbauer, H.; M. Dasyra, K.; Leiton, R.; M. Mazzarella, J.; M. Alexander, D.; Buat, V.; Burgarella, D.; Chary, Ranga‐Ram; Gilli, R.; J. Ivison, R.; Juneau, S.; Le Floc’h, E.; Lutz, D.; Morrison, G.; Mullaney, James; J. Murphy, E.; Pope, A.; Scott, D.; Brodwin, M.; Calzetti, Daniela; J. Césarsky, C.; Charlot, S.; Dole, H.; Eisenhardt, Peter; C. Ferguson, H.; M. Förster Schreiber, N.; T. Frayer, D.; Giavalisco, Mauro; Huynh, Minh; M. Koekemoer, Anton; Papovich, Casey

doi:10.1051/0004-6361/201117239

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GOODS–Herschel: an infrared main sequence for star-forming galaxies

Shared by NobleBlocks on Aug 10, 2011 • 12:00 AM UTC

Authors:

D. Elbaz

Mark Dickinson

Ho Seong Hwang

Abstract

We present the deepest 100 to 500 μm far-infrared observations obtained with the Herschel Space Observatory as part of the GOODS-Herschel key program, and examine the infrared (IR) 3–500 μm spectral energy distributions (SEDs) of galaxies at 0 < z < 2.5, supplemented by a local reference sample from...

Subject

Physics

Astrophysics

Luminous infrared galaxy

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