{"paper":{"title":"A Population of z>2 Far-Infrared Herschel-SPIRE selected Starbursts","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"(10) Cambridge, 11), (11) Dalhousie, (12) Imperial, (13) Colorado, (14) Nottingham, (15) UCI, (16) Virginia Tech, (17) ESO, (18) UKATC, 19), (19) Edinburgh, 20), (20) Oxford, (21) Sussex, (22) MSSL, (23) Bologna, 24), (24) RAL, 25), (25) NASA Ames, 26), (26) CSIRO), (2) MPE, (3) Saclay, 4), (4) IAS, 5), (5) Caltech, 6), (6) JPL, (7) Marseille, (8) UBC, 9), (9) ESAC, A. Conley (13), A. Cooray (15, B. Magnelli (2), C. Bridge (5), C. J. Conselice (14), C. M. Casey (1), D. B. Sanders (1), D. Burgarella (7), D. Farrah (16), D. L. Clements (12), D. Lutz (2), D. Rigopoulou (20, D. Scott (8), E. Chapin (8, E. Hatziminaoglou (17), E. Le Floc'h (3), F. Pozzi (23), G. Magdis (3, I. G. Roseboom (21, I. Valtchanov (9), J. Bock (5, J. D. Vieira (5), J. Wardlow (15) ((1) Hawaii, L. Riguccini (3, M. B\\'ethermin (3, M. J. Page (22), M. Viero (5), N. Seymour (22, R. J. Ivison (18, S. Berta (2), S. C. Chapman (10, S. J. Oliver (21)","submitted_at":"2012-10-17T20:00:05Z","abstract_excerpt":"We present spectroscopic observations for a sample of 36 Herschel-SPIRE 250-500um selected galaxies (HSGs) at 2<z<5 from the Herschel Multi-tiered Extragalactic Survey (HerMES). Redshifts are confirmed as part of a large redshift survey of Herschel-SPIRE-selected sources covering ~0.93deg^2 in six extragalactic legacy fields. Observations were taken with the Keck I Low Resolution Imaging Spectrometer (LRIS) and the Keck II DEep Imaging Multi-Object Spectrograph (DEIMOS). Precise astrometry, needed for spectroscopic follow-up, is determined by identification of counterparts at 24um or 1.4GHz us"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1210.4932","kind":"arxiv","version":2},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}