Publication date: 04 December 2012
Authors: Casey, C.M., et al.
Journal: The Astrophysical Journal
Copyright: The American Astronomical Society
We present spectroscopic observations for a sample of 36 Herschel-SPIRE 250-500 micron selected galaxies (HSGs) at 22 in six extragalactic legacy fields. Observations were taken with the Keck I Low Resolution Imaging Spectrometer (LRIS) and the Keck II DEep Imaging Multi-Object Spectrograph (DEIMOS). Precise astrometry, needed for spectroscopic follow-up, is determined by identification of counterparts at 24 um or 1.4 GHz using a cross-identification likelihood matching method. Individual source luminosities range from log(LIR/LSun)=12.5-13.6 (corresponding to star formation rates 500-9000 MSun/yr, assuming a Salpeter IMF), constituting some of the most intrinsically luminous, distant infrared galaxies yet discovered. We present both individual and composite rest-frame ultraviolet spectra and infrared spectral energy distributions (SEDs). The selection of these HSGs is reproducible and well characterized across large areas of sky in contrast to most z>2 HyLIRGs in the literature which are detected serendipitously or via tailored surveys searching only for high-z HyLIRGs; therefore, we can place lower limits on the contribution of HSGs to the cosmic star formation rate density at (7+/-2)x10-3MSun/yr h3Mpc-3 at z~2.5, which is >10% of the estimated total star formation rate density (SFRD) of the Universe from optical surveys. The contribution at z~4 has a lower limit of 3x10-3MSun/yr h3Mpc-3, ~>20% of the estimated total SFRD. This highlights the importance of extremely infrared-luminous galaxies with high star formation rates to the build-up of stellar mass, even at the earliest epochs.
Link to Publication: http://dx.doi.org/10.1088/0004-637X/761/2/139