Abstract
We present deep Ks83 μJy (the ~80% completeness limit of the Spitzer/GTO 24
μm catalog); 36% of our galaxies have spectroscopic redshifts (mostly
at z~1.5. We
determine the existence of a bump in the redshift distribution at z~1.9,
indicating the presence of a significant population of galaxies with PAH
emission at these redshifts. The 24 μm galaxy population ranges from
sources with intermediate luminosities (1010
Lsolar~1011
Msolar) hyperluminous galaxies
(LIR>1012 Lsolar) at redshifts
z~2-3. Massive star-forming galaxies at redshifts 2500
Msolar yr-1), and some of them are able to
construct a mass of ~1010-1011 Msolar
in a single burst lifetime (~0.01-0.1 Gyr). At lower redshifts z
Original language | English |
---|---|
Pages (from-to) | 727-740 |
Journal | Astrophysical Journal |
Volume | 637 |
DOIs | |
Publication status | Published - 1 Feb 2006 |