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An ALMA Survey of Submilleter Galaxies in the Extended Chandra Deep Field-South : The AGN Fraction and X-Ray Properties of Submillimeter Galaxies

dc.contributor.authorWang, S.X.
dc.contributor.authorBrandt, W. N.
dc.contributor.authorLuo, B.
dc.contributor.authorSmail, I.
dc.contributor.authorAlexander, D.M.
dc.contributor.authorDanielson, A. L. R.
dc.contributor.authorHodge, J. A.
dc.contributor.authorKarim, A.
dc.contributor.authorLehmer, B.D.
dc.contributor.authorSimpson, James
dc.contributor.authorSwinbank, A.M.
dc.contributor.authorWalter, Fabian
dc.contributor.authorWardlow, Julie
dc.contributor.authorXue, Y. Q.
dc.contributor.authorChapman, S.
dc.contributor.authorCoppin, Kristen
dc.contributor.authorDannerbauer, H.
dc.contributor.authorDe Breuck, Carlos
dc.contributor.authorMenten, K. M.
dc.contributor.authorvan der Werf, P.
dc.date.accessioned2014-01-27T14:30:33Z
dc.date.available2014-01-27T14:30:33Z
dc.date.issued2013
dc.identifier.citationWang , S X , Brandt , W N , Luo , B , Smail , I , Alexander , D M , Danielson , A L R , Hodge , J A , Karim , A , Lehmer , B D , Simpson , J , Swinbank , A M , Walter , F , Wardlow , J , Xue , Y Q , Chapman , S , Coppin , K , Dannerbauer , H , De Breuck , C , Menten , K M & van der Werf , P 2013 , ' An ALMA Survey of Submilleter Galaxies in the Extended Chandra Deep Field-South : The AGN Fraction and X-Ray Properties of Submillimeter Galaxies ' , The Astrophysical Journal , vol. 778 , no. 2 , 179 . https://doi.org/10.1088/0004-637X/778/2/179
dc.identifier.issn0004-637X
dc.identifier.otherPURE: 2712482
dc.identifier.otherPURE UUID: 5bb3b189-fa44-416b-b7a4-aa8e01817290
dc.identifier.otherScopus: 84887883158
dc.identifier.otherORCID: /0000-0002-0729-2988/work/30423064
dc.identifier.urihttp://hdl.handle.net/2299/12692
dc.descriptioncopyright American Astronomical Society
dc.description.abstractThe large gas and dust reservoirs of submillimeter galaxies (SMGs) could potentially provide ample fuel to trigger an active galactic nucleus (AGN), but previous studies of the AGN fraction in SMGs have been controversial largely due to the inhomogeneity and limited angular resolution of the available submillimeter surveys. Here we set improved constraints on the AGN fraction and X-ray properties of the SMGs with Atacama Large Millimeter/submillimeter Array (ALMA) and Chandra observations in the Extended Chandra Deep Field-South (E-CDF-S). This study is the first among similar works to have unambiguously identified the X-ray counterparts of SMGs; this is accomplished using the fully submillimeter-identified, statistically reliable SMG catalog with 99 SMGs from the ALMA LABOCA E-CDF-S Submillimeter Surveyen
dc.format.extent25
dc.language.isoeng
dc.relation.ispartofThe Astrophysical Journal
dc.titleAn ALMA Survey of Submilleter Galaxies in the Extended Chandra Deep Field-South : The AGN Fraction and X-Ray Properties of Submillimeter Galaxiesen
dc.contributor.institutionCentre for Astrophysics Research
dc.description.statusPeer reviewed
rioxxterms.versionSMUR
rioxxterms.versionofrecordhttps://doi.org/10.1088/0004-637X/778/2/179
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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