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dc.contributor.authorSymeonidis, M.
dc.contributor.authorGeorgakakis, A.
dc.contributor.authorSeymour, Nick
dc.contributor.authorAuld, R.
dc.contributor.authorBock, J.
dc.contributor.authorBrisbin, D.
dc.contributor.authorBuat, V.
dc.contributor.authorBurgarella, D.
dc.contributor.authorChanial, P.
dc.contributor.authorClements, D.
dc.contributor.authorCooray, A.
dc.contributor.authorEales, S.
dc.contributor.authorFarrah, D.
dc.contributor.authorFranceschini, A.
dc.contributor.authorGlenn, J.
dc.contributor.authorGriffin, M.
dc.contributor.authorHatziminaoglou, E.
dc.contributor.authorIbar, E.
dc.contributor.authorIvison, R.
dc.contributor.authorMortier, A.
dc.contributor.authorOliver, S.
dc.contributor.authorPage, M.
dc.contributor.authorPapageorgiou, A.
dc.contributor.authorPearson, C.
dc.contributor.authorPérez-Fournon, I.
dc.contributor.authorPohlen, M.
dc.contributor.authorRawlings, J.
dc.contributor.authorRaymond, G.
dc.contributor.authorRodighiero, G.
dc.contributor.authorRoseboom, I.
dc.contributor.authorRowan-Robinson, M.
dc.contributor.authorScott, D.
dc.contributor.authorSmith, A.
dc.contributor.authorTugwell, K.
dc.contributor.authorVaccari, M.
dc.contributor.authorVieira, J.
dc.contributor.authorVigroux, L.
dc.contributor.authorWang, L.
dc.contributor.authorWright, G.
dc.date.accessioned2017-01-30T12:05:29Z
dc.date.available2017-01-30T12:05:29Z
dc.date.created2016-01-18T20:00:46Z
dc.date.issued2011
dc.identifier.citationSymeonidis, M. and Georgakakis, A. and Seymour, N. and Auld, R. and Bock, J. and Brisbin, D. and Buat, V. et al. 2011. Herschel/HerMES: The X-ray-infrared correlation for star-forming galaxies at z~1. Monthly Notices of the Royal Astronomical Society. 417 (3): pp. 2239-2252.
dc.identifier.urihttp://hdl.handle.net/20.500.11937/18028
dc.identifier.doi10.1111/j.1365-2966.2011.19405.x
dc.description.abstract

For the first time, we investigate the X-ray/infrared (IR) correlation for star-forming galaxies (SFGs) at z~ 1, using SPIRE submm data from the recently launched Herschel Space Observatory and deep X-ray data from the 2-Ms Chandra Deep Field-North survey. We examine the X-ray/IR correlation in the soft X-ray (SX; 0.5-2keV) and hard X-ray (HX; 2-10keV) bands by comparing our z~ 1 SPIRE-detected SFGs to equivalently IR-luminous (LIR < 1010 L☉) samples in the local/low-redshift Universe. Our results suggest that the X-ray/IR properties of the SPIRE SFGs are on average similar to those of their local counterparts, as we find no evidence for evolution in the LSX/LIR and LHX/LIR ratios with redshift. We note, however, that at all redshifts, both LSX/LIR and LHX/LIR are strongly dependent on IR luminosity, with luminous and ultraluminous IR galaxies (LIRGs and ULIRGs; LIR < 1011 L☉) having up to an order of magnitude lower values than normal IR galaxies (LIR < 1011 L☉). We derive a LSX-LIR relation and confirm the applicability of an existing LHX-LIR relation for both local and distant LIRGs and ULIRGs, consistent with a scenario where X-ray luminosity is correlated with the star formation rate.

dc.titleHerschel/HerMES: The X-ray-infrared correlation for star-forming galaxies at z~1
dc.typeJournal Article
dcterms.source.volume417
dcterms.source.number3
dcterms.source.startPage2239
dcterms.source.endPage2252
dcterms.source.issn0035-8711
dcterms.source.titleMonthly Notices of the Royal Astronomical Society
curtin.note

This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2011 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.

curtin.departmentDepartment of Physics and Astronomy
curtin.accessStatusOpen access


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