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dc.contributor.authorOliver, S. J.
dc.contributor.authorBock, J.
dc.contributor.authorAltieri, B.
dc.contributor.authorAmblard, A.
dc.contributor.authorArumugam, V.
dc.contributor.authorAussel, H.
dc.contributor.authorBabbedge, T.
dc.contributor.authorBeelen, A.
dc.contributor.authorBéthermin, M.
dc.contributor.authorBlain, A.
dc.contributor.authorBoselli, A.
dc.contributor.authorBridge, C.
dc.contributor.authorBrisbin, D.
dc.contributor.authorBuat, V.
dc.contributor.authorBurgarella, D.
dc.contributor.authorCastro-Rodríguez, N.
dc.contributor.authorCava, A.
dc.contributor.authorChanial, P.
dc.contributor.authorCirasuolo, M.
dc.contributor.authorClements, D. L.
dc.contributor.authorConley, A.
dc.contributor.authorConversi, L.
dc.contributor.authorCooray, A.
dc.contributor.authorDowell, C.D.
dc.contributor.authorDubois, E. N.
dc.contributor.authorDwek, E.
dc.contributor.authorDye, S.
dc.contributor.authorEales, S.
dc.contributor.authorElbaz, D.
dc.contributor.authorFarrah, D.
dc.contributor.authorFeltre, A.
dc.contributor.authorFerrero, P.
dc.contributor.authorFiolet, N.
dc.contributor.authorFox, M.
dc.contributor.authorFranceschini, A.
dc.contributor.authorGear, W.
dc.contributor.authorGiovannoli, E.
dc.contributor.authorGlenn, J.
dc.contributor.authorGong, Y.
dc.contributor.authorGonzález Solares, E. A.
dc.contributor.authorGriffin, M.
dc.contributor.authorHalpern, M.
dc.contributor.authorHarwit, M.
dc.contributor.authorHatziminaoglou, E.
dc.contributor.authorHeinis, S.
dc.contributor.authorHurley, P.
dc.contributor.authorHwang, H. S.
dc.contributor.authorHyde, A.
dc.contributor.authorIbar, E.
dc.contributor.authorIlbert, O.
dc.contributor.authorIsaak, K.
dc.contributor.authorIvison, R. J.
dc.contributor.authorLagache, G.
dc.contributor.authorLe Floc'h, E.
dc.contributor.authorLevenson, L.
dc.contributor.authorFaro, B. L.
dc.contributor.authorLu, N.
dc.contributor.authorMadden, S.
dc.contributor.authorMaffei, B.
dc.contributor.authorMagdis, G.
dc.contributor.authorMainetti, G.
dc.contributor.authorMarchetti, L.
dc.contributor.authorMarsden, G.
dc.contributor.authorMarshall, J.
dc.contributor.authorMortier, A. M. J.
dc.contributor.authorNguyen, H.T.
dc.contributor.authorO'Halloran, B.
dc.contributor.authorOmont, A.
dc.contributor.authorPage, M.J.
dc.contributor.authorPanuzzo, P.
dc.contributor.authorPapageorgiou, A.
dc.contributor.authorPatel, H.
dc.contributor.authorPearson, C.P.
dc.contributor.authorPérez-Fournon, I.
dc.contributor.authorPohlen, M.
dc.contributor.authorRawlings, J.I.
dc.contributor.authorRaymond, G.
dc.contributor.authorRigopoulou, D.
dc.contributor.authorRiguccini, L.
dc.contributor.authorRizzo, D.
dc.contributor.authorRodighiero, G.
dc.contributor.authorRoseboom, I.G.
dc.contributor.authorRowan-Robinson, M.
dc.contributor.authorSánchez Portal, M.
dc.contributor.authorSchulz, B.
dc.contributor.authorScott, D.
dc.contributor.authorSeymour, N.
dc.contributor.authorShupe, D. L.
dc.contributor.authorSmith, A.J.
dc.contributor.authorStevens, J. A.
dc.contributor.authorSymeonidis, M.
dc.contributor.authorTrichas, M.
dc.contributor.authorTugwell, K.E.
dc.contributor.authorVaccari, M.
dc.contributor.authorValtchanov, I.
dc.contributor.authorVieira, J. D.
dc.contributor.authorViero, M.
dc.contributor.authorVigroux, L.
dc.contributor.authorWang, L.
dc.contributor.authorWard, R.
dc.contributor.authorWardlow, J.
dc.contributor.authorWright, G.
dc.contributor.authorXu, C. K.
dc.contributor.authorZemcov, M.
dc.date.accessioned2012-08-08T13:00:27Z
dc.date.available2012-08-08T13:00:27Z
dc.date.issued2012-08-01
dc.identifier.citationOliver , S J , Bock , J , Altieri , B , Amblard , A , Arumugam , V , Aussel , H , Babbedge , T , Beelen , A , Béthermin , M , Blain , A , Boselli , A , Bridge , C , Brisbin , D , Buat , V , Burgarella , D , Castro-Rodríguez , N , Cava , A , Chanial , P , Cirasuolo , M , Clements , D L , Conley , A , Conversi , L , Cooray , A , Dowell , C D , Dubois , E N , Dwek , E , Dye , S , Eales , S , Elbaz , D , Farrah , D , Feltre , A , Ferrero , P , Fiolet , N , Fox , M , Franceschini , A , Gear , W , Giovannoli , E , Glenn , J , Gong , Y , González Solares , E A , Griffin , M , Halpern , M , Harwit , M , Hatziminaoglou , E , Heinis , S , Hurley , P , Hwang , H S , Hyde , A , Ibar , E , Ilbert , O , Isaak , K , Ivison , R J , Lagache , G , Le Floc'h , E , Levenson , L , Faro , B L , Lu , N , Madden , S , Maffei , B , Magdis , G , Mainetti , G , Marchetti , L , Marsden , G , Marshall , J , Mortier , A M J , Nguyen , H T , O'Halloran , B , Omont , A , Page , M J , Panuzzo , P , Papageorgiou , A , Patel , H , Pearson , C P , Pérez-Fournon , I , Pohlen , M , Rawlings , J I , Raymond , G , Rigopoulou , D , Riguccini , L , Rizzo , D , Rodighiero , G , Roseboom , I G , Rowan-Robinson , M , Sánchez Portal , M , Schulz , B , Scott , D , Seymour , N , Shupe , D L , Smith , A J , Stevens , J A , Symeonidis , M , Trichas , M , Tugwell , K E , Vaccari , M , Valtchanov , I , Vieira , J D , Viero , M , Vigroux , L , Wang , L , Ward , R , Wardlow , J , Wright , G , Xu , C K & Zemcov , M 2012 , ' The Herschel Multi-tiered Extragalactic Survey: HerMES ' , Monthly Notices of the Royal Astronomical Society , vol. 424 , no. 3 , pp. 1614-1635 . https://doi.org/10.1111/j.1365-2966.2012.20912.x
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 971286
dc.identifier.otherPURE UUID: d0c0675c-ccb3-42e7-8652-49ec7b14e455
dc.identifier.otherBibtex: urn:c7a2df2ac964ca6beefc526e02550f1a
dc.identifier.otherScopus: 84864506579
dc.identifier.urihttp://hdl.handle.net/2299/8815
dc.description.abstractThe Herschel Multi-tiered Extragalactic Survey (HerMES) is a legacy programme designed to map a set of nested fields totalling ∼380 deg2. Fields range in size from 0.01 to ∼20  deg 2, using the Herschel-Spectral and Photometric Imaging Receiver (SPIRE) (at 250, 350 and 500 μm) and the Herschel-Photodetector Array Camera and Spectrometer (PACS) (at 100 and 160 μm), with an additional wider component of 270 deg2 with SPIRE alone. These bands cover the peak of the redshifted thermal spectral energy distribution from interstellar dust and thus capture the reprocessed optical and ultraviolet radiation from star formation that has been absorbed by dust, and are critical for forming a complete multiwavelength understanding of galaxy formation and evolution. The survey will detect of the order of 100 000 galaxies at 5σ in some of the best-studied fields in the sky. Additionally, HerMES is closely coordinated with the PACS Evolutionary Probe survey. Making maximum use of the full spectrum of ancillary data, from radio to X-ray wavelengths, it is designed to facilitate redshift determination, rapidly identify unusual objects and understand the relationships between thermal emission from dust and other processes. Scientific questions HerMES will be used to answer include the total infrared emission of galaxies, the evolution of the luminosity function, the clustering properties of dusty galaxies and the properties of populations of galaxies which lie below the confusion limit through lensing and statistical techniques. This paper defines the survey observations and data products, outlines the primary scientific goals of the HerMES team, and reviews some of the early resultsen
dc.format.extent22
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.rightsEmbargoed
dc.titleThe Herschel Multi-tiered Extragalactic Survey: HerMESen
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.date.embargoedUntil2013-02-01
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
dc.description.versiontypeFinal Accepted Version
dcterms.dateAccepted2012-08-01
rioxxterms.versionAM
rioxxterms.versionofrecordhttps://doi.org/10.1111/j.1365-2966.2012.20912.x
rioxxterms.licenseref.startdate2013-02-01
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue
herts.date.embargo2013-02-01
herts.rights.accesstypeEmbargoed


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