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The host galaxies of X-ray selected active galactic nuclei to z = 2.5: Structure, star formation, and their relationships from CANDELS and Herschel /PACS

dc.creatorRosario, D. J.
dc.creatorMcIntosh, D. H.
dc.creatorvan der Wel, A.
dc.creatorKartaltepe, J.
dc.creatorLang, P.
dc.creatorSantini, P.
dc.creatorWuyts, S.
dc.creatorLutz, D.
dc.creatorRafelski, M.
dc.creatorVillforth, C.
dc.creatorAlexander, D. M.
dc.creatorBauer, F. E.
dc.creatorBell, E. F.
dc.creatorBerta, S.
dc.creatorBrandt, W. N.
dc.creatorConselice, C. J.
dc.creatorDekel, A.
dc.creatorFaber, S. M.
dc.creatorFerguson, H. C.
dc.creatorGenzel, R.
dc.creatorGrogin, N. A.
dc.creatorKocevski, D. D.
dc.creatorKoekemoer, A. M.
dc.creatorKoo, D. C.
dc.creatorLotz, J. M.
dc.creatorMagnelli, B.
dc.creatorMaiolino, R.
dc.creatorMozena, M.
dc.creatorMullaney, J. R.
dc.creatorPapovich, C. J.
dc.creatorPopesso, P.
dc.creatorTacconi, L. J.
dc.creatorTrump, J. R.
dc.creatorAvadhuta, S.
dc.creatorBassett, R.
dc.creatorBell, A.
dc.creatorBernyk, M.
dc.creatorBournaud, F.
dc.creatorCassata, P.
dc.creatorCheung, E.
dc.creatorCroton, D.
dc.creatorDonley, J.
dc.creatorDeGroot, L.
dc.creatorGuedes, J.
dc.creatorHathi, N.
dc.creatorHerrington, J.
dc.creatorHilton, M.
dc.creatorLai, K.
dc.creatorLani, C.
dc.creatorMartig, M.
dc.creatorMcGrath, E.
dc.creatorMutch, S.
dc.creatorMortlock, A.
dc.creatorMcPartland, C.
dc.creatorO’Leary, E.
dc.creatorPeth, M.
dc.creatorPillepich, A.
dc.creatorPoole, G.
dc.creatorSnyder, D.
dc.creatorStraughn, A.
dc.creatorTelford, O.
dc.creatorTonini, C.
dc.creatorWandro, P.
dc.date.accessioned2019-10-09T16:21:51Z
dc.date.available2019-10-09T16:21:51Z
dc.date.issued2015
dc.identifier.issn0004-6361
dc.identifier.issn1432-0746
dc.identifier.urihttps://hdl.handle.net/1969.1/180625
dc.format.extent1en
dc.publisherAstronomy and Astrophysics
dc.relation.ispartof1foldr Import 2019-10-08 Batch 5en
dc.relation.uri10.1051/0004-6361/201423782en
dc.titleThe host galaxies of X-ray selected active galactic nuclei to z = 2.5: Structure, star formation, and their relationships from CANDELS and Herschel /PACSen


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