dc.contributor.author | Roseboom, I. G. | en_US |
dc.contributor.author | Ivison, R. J. | en_US |
dc.contributor.author | Greve, T. R. | en_US |
dc.contributor.author | Amblard, A. | en_US |
dc.contributor.author | Arumugam, V. | en_US |
dc.contributor.author | Auld, R. | en_US |
dc.contributor.author | Aussel, H. | en_US |
dc.contributor.author | Bethermin, M. | en_US |
dc.contributor.author | Blain, A. | en_US |
dc.contributor.author | Bock, J. | en_US |
dc.contributor.author | Boselli, A. | en_US |
dc.contributor.author | Brisbin, D. | en_US |
dc.contributor.author | Buat, V. | en_US |
dc.contributor.author | Burgarella, D. | en_US |
dc.contributor.author | Castro-Rodriguez, N. | en_US |
dc.contributor.author | Cava, A. | en_US |
dc.contributor.author | Chanial, P. | en_US |
dc.contributor.author | Chapin, E. | en_US |
dc.contributor.author | Chapman, S. | en_US |
dc.contributor.author | Clements, D. L. | en_US |
dc.contributor.author | Conley, A. | en_US |
dc.contributor.author | Conversi, L. | en_US |
dc.contributor.author | Cooray, A. | en_US |
dc.contributor.author | Dowell, C. D. | en_US |
dc.contributor.author | Dunlop, J. S. | en_US |
dc.contributor.author | Dwek, E. | en_US |
dc.contributor.author | Eales, S. | en_US |
dc.contributor.author | Elbaz, D. | en_US |
dc.contributor.author | Farrah, D. | en_US |
dc.contributor.author | Franceschini, A. | en_US |
dc.contributor.author | Glenn, J. | en_US |
dc.contributor.author | Griffin, M. | en_US |
dc.contributor.author | Halpern, M. | en_US |
dc.contributor.author | Hatziminaoglou, E. | en_US |
dc.contributor.author | Ibar, E. | en_US |
dc.contributor.author | Isaak, K. | en_US |
dc.contributor.author | Lagache, G. | en_US |
dc.contributor.author | Levenson, L. | en_US |
dc.contributor.author | Lu, N. | en_US |
dc.contributor.author | Madden, S. | en_US |
dc.contributor.author | Maffei, B. | en_US |
dc.contributor.author | Mainetti, G. | en_US |
dc.contributor.author | Marchetti, L. | en_US |
dc.contributor.author | Marsden, G. | en_US |
dc.contributor.author | Morrison, G. | en_US |
dc.contributor.author | Mortier, A. M. J. | en_US |
dc.contributor.author | Nguyen, H. T. | en_US |
dc.contributor.author | O'Halloran, B. | en_US |
dc.contributor.author | Oliver, S. J. | en_US |
dc.contributor.author | Omont, A. | en_US |
dc.contributor.author | Page, M. J. | en_US |
dc.contributor.author | Panuzzo, P. | en_US |
dc.contributor.author | Papageorgiou, A. | en_US |
dc.contributor.author | Pearson, C. P. | en_US |
dc.contributor.author | Perez-Fournon, I. | en_US |
dc.contributor.author | Pohlen, M. | en_US |
dc.contributor.author | Rawlings, J. I. | en_US |
dc.contributor.author | Raymond, G. | en_US |
dc.contributor.author | Rigopoulou, D. | en_US |
dc.contributor.author | Rizzo, D. | en_US |
dc.contributor.author | Rodighiero, G. | en_US |
dc.contributor.author | Rowan-Robinson, M. | en_US |
dc.contributor.author | Schulz, B. | en_US |
dc.contributor.author | Scott, Douglas | en_US |
dc.contributor.author | Seymour, N. | en_US |
dc.contributor.author | Shupe, D. L. | en_US |
dc.contributor.author | Smith, A. J. | en_US |
dc.contributor.author | Stevens, J. A. | en_US |
dc.contributor.author | Symeonidis, M. | en_US |
dc.contributor.author | Trichas, M. | en_US |
dc.contributor.author | Tugwell, K. E. | en_US |
dc.contributor.author | Vaccari, M. | en_US |
dc.contributor.author | Valtchanov, I. | en_US |
dc.contributor.author | Vieira, J. D. | en_US |
dc.contributor.author | Viero, M. P. | en_US |
dc.contributor.author | Vigroux, L. | en_US |
dc.contributor.author | Wardlow, J. | en_US |
dc.contributor.author | Wang, L. | en_US |
dc.contributor.author | Wright, G. | en_US |
dc.contributor.author | Xu, C. K. | en_US |
dc.contributor.author | Zemcov, M. | en_US |
dc.date.accessioned | 2014-03-12T19:20:58Z | |
dc.date.available | 2014-03-12T19:20:58Z | |
dc.date.issued | 2011-09-13 | en_US |
dc.identifier.citation | Roseboom, I. G., R. J. Ivison, T. R. Greve, A. Amblard, et al. 2011. "The Herschel Multi-Tiered Extragalactic Survey: SPIRE-mm Photometric Redshifts." Monthly Notices of the Royal Astronomical Society 419:2758. | en_US |
dc.identifier.issn | 0035-8711 | |
dc.identifier.uri | http://hdl.handle.net/10222/45420 | |
dc.identifier.uri | http://dx.doi.org/10.1111/j.1365-2966.2011.19827.x | |
dc.description.abstract | We investigate the potential of submm-mm and submm-mm-radio photometric redshifts using a sample of mm-selected sources as seen at 250, 350 and 500 {\mu}m by the SPIRE instrument on Herschel. From a sample of 63 previously identified mm-sources with reliable radio identifications in the GOODS-N and Lockman Hole North fields 46 (73 per cent) are found to have detections in at least one SPIRE band. We explore the observed submm/mm colour evolution with redshift, finding that the colours of mm-sources are adequately described by a modified blackbody with constant optical depth {\tau} = ({\nu}/{\nu}0)^{\beta} where {\beta} = +1.8 and {\nu}0 = c/100 {\mu}m. We find a tight correlation between dust temperature and IR luminosity. Using a single model of the dust temperature and IR luminosity relation we derive photometric redshift estimates for the 46 SPIRE detected mm-sources. Testing against the 22 sources with known spectroscopic, or good quality optical/near-IR photometric, redshifts we find submm/mm photometric redshifts offer a redshift accuracy of |z|/(1+z) = 0.16 (= 0.51). Including constraints from the radio-far IR correlation the accuracy is improved to |z|/(1 + z) = 0.15 (= 0.45). We estimate the redshift distribution of mm-selected sources finding a significant excess at z > 3 when compared to ~ 850 {\mu}m selected samples. | en_US |
dc.relation.ispartof | Monthly Notices of the Royal Astronomical Society | |
dc.title | The Herschel Multi-Tiered Extragalactic Survey: SPIRE-mm Photometric Redshifts | en_US |
dc.title.alternative | arXiv:1109.2887 [astro-ph] | en_US |
dc.type | article | en_US |
dc.identifier.volume | 419 | |
dc.identifier.startpage | 2758 | en_US |