The complex physics of dusty star-forming galaxies at high redshifts as revealed by herschel and Spitzer
Astrophysical Journal 762:2 (2013)
Authors:
B Lo Faro, A Franceschini, M Vaccari, L Silva, G Rodighiero, S Berta, J Bock, D Burgarella, V Buat, A Cava, DL Clements, A Cooray, D Farrah, A Feltre, EAG Solares, P Hurley, D Lutz, G Magdis, B Magnelli, L Marchetti, SJ Oliver, MJ Page, P Popesso, F Pozzi, D Rigopoulou, M Rowan-Robinson, IG Roseboom, D Scott, AJ Smith, M Symeonidis, L Wang, S Wuyts
Abstract:
We combine far-infrared photometry from Herschel (PEP/HerMES) with deep mid-infrared spectroscopy from Spitzer to investigate the nature and the mass assembly history of a sample of 31 luminous and ultraluminous infrared galaxies ((U)LIRGs) at z &thk 1 and 2 selected in GOODS-S with 24 μm fluxes between 0.2 and 0.5 mJy. We model the data with a self-consistent physical model (GRASIL) which includes a state-of-the-art treatment of dust extinction and reprocessing. We find that all of our galaxies appear to require massive populations of old (>1 Gyr) stars and, at the same time, to host a moderate ongoing activity of star formation (SFR ≤ 100M yr-1). The bulk of the stars appear to have been formed a few Gyr before the observation in essentially all cases. Only five galaxies of the sample require a recent starburst superimposed on a quiescent star formation history. We also find discrepancies between our results and those based on optical-only spectral energy distribution (SED) fitting for the same objects; by fitting their observed SEDs with our physical model we find higher extinctions (by ΔAV &thk 0.81 and 1.14) and higher stellar masses (by Δlog(M) &thk 0.16 and 0.36 dex) for z &thk 1 and z &thk 2 (U)LIRGs, respectively. The stellar mass difference is larger for the most dust-obscured objects. We also find lower SFRs than those computed from LIR using the Kennicutt relation due to the significant contribution to the dust heating by intermediate-age stellar populations through "cirrus" emission (&thk73% and &thk66% of the total LIR for z &thk 1 and z &thk 2 (U)LIRGs, respectively). © 2013. The American Astronomical Society. All rights reserved..
