A Population of z > 2 Far-infrared Herschel-SPIRE-selected Starbursts
Berta, S.; Magnelli, B.; Lutz, D.; Pozzi, F.; Riguccini, L.; Valtchanov, I.; Ivison, R. J.; Sanders, D. B.; Clements, D. L.; Béthermin, M.; Burgarella, D.; Hatziminaoglou, E.; Bock, J.; Cooray, A.; Farrah, D.; Oliver, S. J.; Page, M. J.; Rigopoulou, D.; Roseboom, I. G.; Conley, A.; Magdis, G.; Seymour, N.; Vieira, J. D.; Conselice, C. J.; Chapman, S. C.; Bridge, C.; Scott, Douglas; Chapin, E.; Viero, M.; Casey, C. M.; Wardlow, J.; le Floc'h, E.
United States, Germany, France, Canada, Spain, United Kingdom, Italy, Australia
Abstract
We present spectroscopic observations for a sample of 36 Herschel-SPIRE 250-500 μm selected galaxies (HSGs) at 2 < z < 5 from the Herschel Multi-tiered Extragalactic Survey. Redshifts are confirmed as part of a large redshift survey of Herschel-SPIRE-selected sources covering ~0.93 deg2 in six extragalactic legacy fields. Observations were taken with the Keck I Low Resolution Imaging Spectrometer and the Keck II DEep Imaging Multi-Object Spectrograph. Precise astrometry, needed for spectroscopic follow-up, is determined by identification of counterparts at 24 μm or 1.4 GHz using a cross-identification likelihood matching method. Individual source luminosities range from log (L IR/L ⊙) = 12.5-13.6 (corresponding to star formation rates (SFRs) 500-9000 M ⊙ yr-1, assuming a Salpeter initial mass function), constituting some of the most intrinsically luminous, distant infrared galaxies discovered thus far. We present both individual and composite rest-frame ultraviolet spectra and infrared spectral energy distributions. The selection of these HSGs is reproducible and well characterized across large areas of the 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 (SFRD) at (7 ± 2) × 10-3 M ⊙ yr-1 h 3 Mpc-3 at z ~ 2.5, which is >10% of the estimated total SFRD of the universe from optical surveys. The contribution at z ~ 4 has a lower limit of 3 × 10-3 M ⊙ yr-1 h 3 Mpc-3, gsim20% of the estimated total SFRD. This highlights the importance of extremely infrared-luminous galaxies with high SFRs to the buildup of stellar mass, even at the earliest epochs.