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dc.contributor.authorPenner, K.
dc.contributor.authorPope, A.
dc.contributor.authorChapin, E.L.
dc.contributor.authorGreve, T.R.
dc.contributor.authorBertoldi, F.
dc.contributor.authorBrodwin, M.
dc.contributor.authorChary, R.
dc.contributor.authorConselice, C. J.
dc.contributor.authorCoppin, Kristen
dc.contributor.authorGiavalisco, M.
dc.contributor.authorHughes, D.H.
dc.contributor.authorIvison, R.J.
dc.contributor.authorPerera, T.
dc.contributor.authorScott, D.
dc.contributor.authorScott, K.
dc.contributor.authorWilson, G.
dc.date.accessioned2014-01-23T16:00:32Z
dc.date.available2014-01-23T16:00:32Z
dc.date.issued2011-02-01
dc.identifier.citationPenner , K , Pope , A , Chapin , E L , Greve , T R , Bertoldi , F , Brodwin , M , Chary , R , Conselice , C J , Coppin , K , Giavalisco , M , Hughes , D H , Ivison , R J , Perera , T , Scott , D , Scott , K & Wilson , G 2011 , ' Origins of the extragalactic background at 1 mm from a combined analysis of the AzTEC and MAMBO data in GOODS-N ' Monthly Notices of the Royal Astronomical Society , vol. 410 , no. 4 , pp. 2749-2759 . https://doi.org/10.1111/j.1365-2966.2010.17650.x
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 2713586
dc.identifier.otherPURE UUID: 986cffca-701f-4be8-ab12-b92ac17619c8
dc.identifier.otherScopus: 78751619870
dc.identifier.otherORCID: /0000-0002-0729-2988/work/30423083
dc.identifier.urihttp://hdl.handle.net/2299/12664
dc.description.abstractWe present a study of the cosmic infrared background, which is a measure of the dust-obscured activity in all galaxies in the Universe. We venture to isolate the galaxies responsible for the background at 1 mm; with spectroscopic and photometric redshifts we constrain the redshift distribution of these galaxies. We create a deep 1.16 mm map (σ∼ 0.5 mJy) by combining the AzTEC 1.1 mm and MAMBO 1.2 mm data sets in the Great Observatories Origins Deep Survey North (GOODS-N) region. This combined map contains 41 secure detections, 13 of which are new. By averaging the 1.16 mm flux densities of individually undetected galaxies with 24 μm flux densities >25 μJy, we resolve 31-45 per cent of the 1.16 mm background. Repeating our analysis on the SCUBA 850 μm map, we resolve a higher percentage (40-64 per cent) of the 850 μm background. A majority of the background resolved (attributed to individual galaxies) at both wavelengths comes from galaxies at z > 1.3. If the ratio of the resolved submillimetre to millimetre background is applied to a reasonable scenario for the origins of the unresolved submillimetre background, 60-88 per cent of the total 1.16 mm background comes from galaxies at z > 1.3.en
dc.format.extent11
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.rights/dk/atira/pure/core/openaccesspermission/open
dc.titleOrigins of the extragalactic background at 1 mm from a combined analysis of the AzTEC and MAMBO data in GOODS-Nen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.contributor.institutionCentre for Astrophysics Research
dc.description.statusPeer reviewed
dc.identifier.urlhttp://www.scopus.com/inward/record.url?scp=78751619870&partnerID=8YFLogxK
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
dc.description.versiontypeSubmitted Version
rioxxterms.versionSMUR
rioxxterms.versionofrecordhttps://doi.org/10.1111/j.1365-2966.2010.17650.x
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue
herts.rights.accesstyperestrictedAccess


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