About: The SCUBA-2 Cosmology Legacy Survey: demographics of the 450-μm population

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About: The SCUBA-2 Cosmology Legacy Survey: demographics of the 450-μm population Goto Sponge NotDistinct Permalink

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scholarly article by I. G. Roseboom et al published September 2013 in Monthly Notices of the Royal Astronomical Society

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description	wetenschappelijk artikel (nl) наукова стаття, опублікована у вересні 2013 (uk) article scientifique publié en 2013 (fr) im September 2013 veröffentlichter wissenschaftlicher Artikel (de) scholarly article by I. G. Roseboom et al published September 2013 in Monthly Notices of the Royal Astronomical Society (en)
publication date	wds:Q56550699-2AFD4D90-BD84-45D9-9C17-03EB16856CC2
publication date	2013-09-01 00:00:00Z (xsd:dateTime)
language of work or name	wds:Q56550699-313E8674-77AD-4559-88FC-1D61A53AB16C
language of work or name	English
cites work	wds:Q56550699-022CB416-F388-4DDF-BC00-B07EE8651FDB wds:Q56550699-02CA5436-A620-47BC-A04F-6216DA70A670 wds:Q56550699-0622783A-68DE-45E4-BE2F-8ACC92592023 wds:Q56550699-0D4D4B4E-BA59-454E-B5DC-B4C0AC917676 wds:Q56550699-0D955EFB-DA6C-4BA3-9B15-FD0D0AE19F32 wds:Q56550699-0E4EE31C-D9FC-4DC8-8F97-97CB604191ED wds:Q56550699-0EC58C30-1262-4A59-9E7B-A33E460C7113 wds:Q56550699-1232ADA8-0983-44C6-9BC4-1BCDD25F81C8 wds:Q56550699-14C0109E-5FDA-4540-8F57-2DBF8B67AEEC wds:Q56550699-1CD2991E-380A-41A3-B34C-DD599B39D0FC wds:Q56550699-1E4A855A-7B84-415E-B1DA-52A18A33968E wds:Q56550699-1E5D678B-7960-4804-85EE-6902CC229D76 wds:Q56550699-20C3C79C-9052-43D7-96F5-E843B4204C8C wds:Q56550699-23698B19-B326-4911-A8CE-6B5404A791A1 wds:Q56550699-3078A897-B076-4816-8F5D-54B279D2B0AA wds:Q56550699-419F95F4-1E3C-4DFC-AD7A-809EB125ABBD wds:Q56550699-428E2484-0BA4-44EA-A516-BF99CCA8C1D0 wds:Q56550699-47ECF69C-D1D8-485A-B71F-000A35DB756C wds:Q56550699-487F7820-050B-4EE8-806E-CF37714DB151 wds:Q56550699-4A7EC5B3-97E6-42B5-8526-C7BD26DDBED2 wds:Q56550699-52CD5405-81FE-4422-B44A-45914AEB19C1 wds:Q56550699-55F835BD-934B-44E5-BCC5-529A63FF229D wds:Q56550699-5764E253-4C56-4850-868F-5EE45527686C wds:Q56550699-5CF37142-24A7-4A17-89C9-0EE023839790 wds:Q56550699-5DD3B639-8D37-4667-9DE5-DD591897841C wds:Q56550699-5E057088-F82F-4DFF-BFDC-1374FAAAA316 wds:Q56550699-6D2594D6-FE3C-489E-A88E-868F0F42E7FC wds:Q56550699-6FF6C934-0483-4F45-B3AC-1064FBFFFBB5 wds:Q56550699-741D7B3B-E0CC-4B77-ADA4-A197040F654B wds:Q56550699-760EEF95-7C89-479B-81EC-2CD877361422 wds:Q56550699-77FC581D-5A49-4F1D-AE3A-2EA0BB440FA5 wds:Q56550699-78C148A4-2191-44BC-9F6E-80996B955957 wds:Q56550699-7A0139DE-5AF2-47A1-B7E9-BF39A6D96D33 wds:Q56550699-7EE54964-9476-4B5E-AC84-AF6F99D04B9F wds:Q56550699-86C5E270-6141-4DE4-908E-CB35E3D81AD2 wds:Q56550699-8E062720-59F9-4DF3-965A-FD6840BE5E66 wds:Q56550699-8F7FE070-EA82-4283-8254-58BB1B7A19A7 wds:Q56550699-9EDEB173-C8CA-4747-8F87-C860F5869162 wds:Q56550699-A0812C0B-4CB3-4D46-B32F-9F224EE90C5B wds:Q56550699-A26C54C5-5B1E-492B-9A60-621C87ECE087 wds:Q56550699-A5697C98-38BD-493D-9D19-1824D1B7B048 wds:Q56550699-A6A76588-E51F-49B7-9FEE-66ECCB3A532F wds:Q56550699-B36A4CCE-84A3-4038-90FC-406A5F1DAA8C wds:Q56550699-B7F7D53C-64D8-4B0F-8DC3-68C6EE99CC0F wds:Q56550699-C2A96738-78D0-4EBB-916B-51F45FE4C53F wds:Q56550699-C9A7E68C-B667-4515-AC2A-7FF34E83653B wds:Q56550699-CD5DF2D2-E617-4901-86F9-407166E8F9F4 wds:Q56550699-CF10D0E0-43FE-440B-B48B-36F436146D1E wds:Q56550699-D5F090D0-BE47-4560-995C-6866D2D54040 wds:Q56550699-D64BA0CF-61B5-44A2-8DAE-181C84EE6B8C wds:Q56550699-D73B5887-C8DA-44FE-86D0-A1C1DBF8B765 wds:Q56550699-D8FB45DB-EF28-4622-8F0C-EAA0DF4BEAF8 wds:Q56550699-DA079115-D56A-4482-9598-1270B92DD2FC wds:Q56550699-DB08C544-17E5-4646-8FDE-BF92E61812D8 wds:Q56550699-DDAA9E31-A93C-47C4-8270-629941694E98 wds:Q56550699-E3F3F267-7F10-4D4C-AE4E-107EFBB3A291 wds:Q56550699-E88117BF-74FB-4B3C-B65D-E2706AEC450A wds:Q56550699-E965B303-6CBF-4EED-A5B4-EFAC09845B3C wds:Q56550699-F97419BE-0F7D-47EB-A81C-84D49261F2CB wds:Q56550699-F9E9E10A-460D-410B-82DD-24C0FD56EEED wds:Q56550699-FC666179-CDFC-44ED-8E39-F0E795207C9C
cites work	Inference from Iterative Simulation Using Multiple Sequences TheHerschel-SPIRE instrument and its in-flight performance Submillimetre galaxies reside in dark matter haloes with masses greater than 3 × 10¹¹ solar masses HerMES: deep galaxy number counts from a P(D) fluctuation analysis of SPIRE Science Demonstration Phase observations HerMES: deep number counts at 250 μm, 350 μm and 500 μm in the COSMOS and GOODS-N fields and the build-up of the cosmic infrared background HerMES: SPIRE galaxy number counts at 250, 350, and 500 μm CANDELS: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey CANDELS: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey--The Hubble Space Telescope observations, imaging data products, and mosaics Galactic Stellar and Substellar Initial Mass Function HerMES: Halo occupation number and bias properties of dusty galaxies from angular clustering measurements An ALMA survey of submillimetre galaxies in the Extended Chandra Deep Field South: high-resolution 870 μm source counts SCUBA-2: the 10 000 pixel bolometer camera on the James Clerk Maxwell Telescope The SCUBA-2 Cosmology Legacy Survey: blank-field number counts of 450-μm-selected galaxies and their contribution to the cosmic infrared background A Herschel view of the far-infrared properties of submillimetre galaxies Integral field spectroscopy of2.0<z<2.7submillimetre galaxies: gas morphologies and kinematics A joint analysis of BLAST 250-500 μm and LABOCA 870 μm observations in the Extended Chandra Deep Field-South The stellar mass content of submillimeter-selected galaxies AzTEC half square degree survey of the SHADES fields â I. Maps, catalogues and source counts The Large Apex BOlometer Camera survey of the Extended Chandra Deep Field South The SCUBA HAlf Degree Extragalactic Survey - III. Identification of radio and mid-infrared counterparts to submillimetre galaxies zCOSMOS: A Large VLT/VIMOS Redshift Survey Covering 0 <z< 3 in the COSMOS Field A Redshift Survey of the Submillimeter Galaxy Population The SCUBA Half-Degree Extragalactic Survey -- I. Survey motivation, design and data processing A Deep Submillimeter Survey of Lensing Clusters: A New Window on Galaxy Formation and Evolution Evolution of dust temperature of galaxies through cosmic time as seen by Herschel Herschel unveils a puzzling uniformity of distant dusty galaxies The Herschel Multi-Tiered Extragalactic Survey: source extraction and cross-identifications in confusion-dominated SPIRE images An AzTEC 1.1 mm survey of the GOODS-N field - II. Multiwavelength identifications and redshift distribution BLAST: resolving the cosmic submillimeter background

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