H-ATLAS: estimating redshifts of Herschel sources from sub-mm fluxes
Valtchanov, I.; Ivison, R. J.; Scott, D.; Cooray, A.; Ibar, E.; Lapi, A.; Krips, M.; De Zotti, G.; Baes, M.; Baker, A. J.; Dariush, A.; Dunne, L.; Dye, S.; Eales, S.; Frayer, D.; Harris, A. I.; Hopwood, R.; Maddox, S.; Michałowski, M. J.; Rosenman, M.; Valiante, E.; van der Werf, P.; Vieira, J. D.; Gomez, H. L.; Aguirre, J. E.; Bradford, C. M.; Bourne, N.; Gonzalez-Nuevo, J.; Lupu, R. E.; Jarvis, M.; Clark, C. J. R.; Pearson, E. A.
United Kingdom, New Zealand, Spain, United States, Belgium, Italy, France, Canada, Netherlands
Abstract
Upon its completion, the Herschel Astrophysics Terahertz Large Area Survey (H-ATLAS) will be the largest sub-millimetre survey to date, detecting close to half-a-million sources. It will only be possible to measure spectroscopic redshifts for a small fraction of these sources. However, if the rest-frame spectral energy distribution (SED) of a typical H-ATLAS source is known, this SED and the observed Herschel fluxes can be used to estimate the redshifts of the H-ATLAS sources without spectroscopic redshifts. In this paper, we use a sub-set of 40 H-ATLAS sources with previously measured redshifts in the range 0.5 < z < 4.2 to derive a suitable average template for high-redshift H-ATLAS sources. We find that a template with two dust components (Tc = 23.9 K, Th = 46.9 K and ratio of mass of cold dust to mass of warm dust of 30.1) provides a good fit to the rest-frame fluxes of the sources in our calibration sample. We use a jackknife technique to estimate the accuracy of the redshifts estimated with this template, finding a root mean square of Δz/(1 + z) = 0.26. For sources for which there is prior information that they lie at z > 1, we estimate that the rms of Δz/(1 + z) = 0.12. We have used this template to estimate the redshift distribution for the sources detected in the H-ATLAS equatorial fields, finding a bimodal distribution with a mean redshift of 1.2, 1.9 and 2.5 for 250, 350 and 500 μm selected sources, respectively.