Cosmic evolution of submillimeter galaxies and their contribution to
  stellar mass assembly
  The nature of galaxies selected at submillimeter wavelengths (SMGs, S_850 > 3
mJy), some of the bolometrically most luminous objects at high redshifts, is
still elusive. In particular their star formation histories and source of
emission are not accurately constrained. In this paper we introduce a new
approach to analyse the SMG data. Namely, we present the first self-consistent
UV-to-radio spectral energy distribution fits of 76 SMGs with spectroscopic
redshifts using all photometric datapoints from ultraviolet to radio
simultaneously. We find that they are highly star-forming (median star
formation rate 713 MSun yr^-1 for SMGs at z>0.5), moderately dust-obscured
(median A_V~2 mag), hosting significant stellar populations (median stellar
mass 3.7x10^11 MSun) of which only a minor part has been formed in the ongoing
starburst episode. This implies that in the past, SMGs experienced either
another starburst episode or merger with several galaxies. The properties of
SMGs suggest that they are progenitors of present-day elliptical galaxies. We
find that these bright SMGs contribute significantly to the cosmic star
formation rate density (~20%) and stellar mass density (~30-50%) at redshifts
2-4. Using number counts at low fluxes we find that as much as 80% of the
cosmic star formation at these redshifts took place in SMGs brighter than 0.1
mJy. We find evidence that a linear infrared-radio correlation holds for SMGs
in an unchanged form up to redshift of 3.6, though its normalization is offset
from the local relation by a factor of ~2.1 towards higher radio luminosities.
We present a compilation of photometry data of SMGs and determinations of
cosmic SFR and stellar mass densities.
