Paper detail

Spectroscopic Characterisation of 250um-Selected Hyper-Luminous Star Forming Galaxies

We present near-infrared spectroscopic observations from VLT ISAAC of thirteen 250μm-luminous galaxies in the CDF-S, seven of which have confirmed redshifts which average to <z > = 2.0 \pm 0.4. Another two sources of the 13 have tentative z > 1 identifications. Eight of the nine redshifts were identified with Hα detection in H- and K-bands, three of which are confirmed redshifts from previous spectroscopic surveys. We use their near-IR spectra to measure Hα line widths and luminosities, which average to 415 \pm 20 km/s and 3 \times 10^35 W (implying SFR(Hα)~200 M_\odot /yr), both similar to the Hα properties of SMGs. Just like SMGs, 250 μm-luminous galaxies have large Hα to far-infrared (FIR) extinction factors such that the Hα SFRs underestimate the FIR SFRs by ~8-80 times. Far-infrared photometric points from observed 24μm through 870μm are used to constrain the spectral energy distributions (SEDs) even though uncertainty caused by FIR confusion in the BLAST bands is significant. The population has a mean dust temperature of Td = 52 \pm 6 K, emissivity β = 1.73 \pm 0.13, and FIR luminosity LFIR = 3 \times 10^13 L_\odot. Although selection at 250μm allows for the detection of much hotter dust dominated HyLIRGs than SMG selection (at 850μm), we do not find any >60 K 'hot-dust' HyLIRGs. We have shown that near-infrared spectroscopy combined with good photometric redshifts is an efficient way to spectroscopically identify and characterise these rare, extreme systems, hundreds of which are being discovered by the newest generation of IR observatories including the Herschel Space Observatory.