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dc.contributor.authorBourne, N.
dc.contributor.authorMaddox, S. J.
dc.contributor.authorDunne, L.
dc.contributor.authorDye, S.
dc.contributor.authorEales, S.
dc.contributor.authorHoyos, C.
dc.contributor.authorGonzalez-Nuevo, J.
dc.contributor.authorSmith, D. J. B.
dc.contributor.authorValiante, E.
dc.contributor.authorde Zotti, G.
dc.contributor.authorIvison, R. J.
dc.contributor.authorRowlands, K.
dc.date.accessioned2014-12-08T16:01:05Z
dc.date.available2014-12-08T16:01:05Z
dc.date.issued2014-10-21
dc.identifier157833912
dc.identifier95de29b1-f9c8-4d9f-bd8d-fea38cc48c2e
dc.identifier000342926300070
dc.identifier000342926300070
dc.identifier84924586522
dc.identifier.citationBourne , N , Maddox , S J , Dunne , L , Dye , S , Eales , S , Hoyos , C , Gonzalez-Nuevo , J , Smith , D J B , Valiante , E , de Zotti , G , Ivison , R J & Rowlands , K 2014 , ' Colour matters : the effects of lensing on the positional offsets between optical and submillimetre galaxies in Herschel*-ATLAS ' , Monthly Notices of the Royal Astronomical Society , vol. 444 , no. 2 , pp. 1884-1892 . https://doi.org/10.1093/mnras/stu1582en
dc.identifier.issn0035-8711
dc.identifier.urihttps://hdl.handle.net/10023/5898
dc.descriptionNB acknowledges support from the EC FP7 SPACE project ASTRODEEP (Ref. no. 312725). JGN acknowledges financial support from the Spanish CSIC for a JAE-DOC fellowship, co-funded by the European Social Fund, by the Spanish Ministerio de Ciencia e Innovacion, AYA2012-39475-C02-01, and Consolider-Ingenio 2010, CSD2010-00064, projects. LD, SJM, and RJI acknowledge support from the European Research Council (ERC) in the form of Advanced Investigator Program, cosmicism.en
dc.description.abstractWe report an unexpected variation in the positional offset distributions between Herschel-Astrophysical Terahertz Large Area Survey (H-ATLAS) submillimetre (submm) sources and their optical associations, depending on both 250-μm signal-to-noise ratio and 250/350-μm colour. We show that redder and brighter submm sources have optical associations with a broader distribution of positional offsets than would be expected if these offsets were due to random positional errors in the source extraction. The observation can be explained by two possible effects: either red submm sources trace a more clustered population than blue ones, and their positional errors are increased by confusion, or red submm sources are generally at high redshifts and are frequently associated with low-redshift lensing structures which are identified as false counterparts. We perform various analyses of the data, including the multiplicity of optical associations, the redshift and magnitude distributions in H-ATLAS in comparison to HerMES, and simulations of weak lensing, and we conclude that the effects are most likely to be explained by widespread weak lensing of Herschel-SPIRE sources by foreground structures. This has important consequences for counterpart identification and derived redshift distributions and luminosity functions of submm surveys.
dc.format.extent9
dc.format.extent477527
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Societyen
dc.subjectGravitational lensing: weaken
dc.subjectGalaxies: statisticsen
dc.subjectSubmillimetre: galaxiesen
dc.subjectScience demonstration phaseen
dc.subjectDigital sky surveyen
dc.subjectDeep field-Southen
dc.subjectStrongly lensed galaxiesen
dc.subjectRedshift distributionen
dc.subjectExtragalactic surveyen
dc.subjectCross correlationen
dc.subjectSource countsen
dc.subjectPhotometric redshiftsen
dc.subjectSource catalogen
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.subject.lccQBen
dc.subject.lccQCen
dc.titleColour matters : the effects of lensing on the positional offsets between optical and submillimetre galaxies in Herschel*-ATLASen
dc.typeJournal articleen
dc.contributor.institutionUniversity of St Andrews. School of Physics and Astronomyen
dc.identifier.doi10.1093/mnras/stu1582
dc.description.statusPeer revieweden


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