The first ISO ERO: A dusty quasar at z = 1.5

dc.contributor.authorPierre, M.en
dc.contributor.authorLidman, C.en
dc.contributor.authorHunstead, R.en
dc.contributor.authorAlloin, D.en
dc.contributor.authorCasali, M.en
dc.contributor.authorCesarsky, C.en
dc.contributor.authorChanial, P.en
dc.contributor.authorDuc, P. -A.en
dc.contributor.authorFadda, D.en
dc.contributor.authorFlores, H.en
dc.contributor.authorMadden, S.en
dc.contributor.authorVigroux, L.en
dc.date.accessioned2026-01-01T13:41:55Z
dc.date.available2026-01-01T13:41:55Z
dc.date.issued2001-06-01en
dc.description.abstractWe report the discovery of an extremely red object (ERO) in a medium-deep ISOCAM extragalactic survey. The object is also a radio source. Subsequent VLT NIR spectroscopy revealed a prominent Hα line giving a redshift of 1.5. We present the spectrum and photometric data points and discuss evidence that ISO J1324-2016 is a quasar harbouring a significant amount of very hot dust. Based on observations collected at the ISO Observatory, Canada-France-Hawaii Telescope, Australia Telescope Compact Array, UKIRT, ROSAT and the European Southern Observatory (prg: 58.E-0885, 61.B-0369, 265.B-5005).en
dc.description.statusPeer-revieweden
dc.identifier.issn0004-6361en
dc.identifier.otherRIS:urn:E2BC80D75F49E9B00D102828AD70E0F0en
dc.identifier.scopus0035373080en
dc.identifier.urihttps://hdl.handle.net/1885/733800732
dc.language.isoenen
dc.sourceAstronomy and Astrophysicsen
dc.subjectINFRARED: GALAXIESen
dc.subjectQUASARS: GENERALen
dc.subjectGALAXIES: STARBURSTen
dc.subjectQUASAR: INDIVIDUAL: ISO J1324-2016en
dc.subjectAstrophysicsen
dc.titleThe first ISO ERO: A dusty quasar at z = 1.5en
dc.typeJournal articleen
dspace.entity.typePublicationen
local.bibliographicCitation.lastpageL49en
local.bibliographicCitation.startpageL45en
local.contributor.affiliationLidman, C.; RSAA Academic Program, Research School of Astronomy & Astrophysics, ANU College of Science and Medicine, The Australian National Universityen
local.identifier.citationvolume372en
local.identifier.doi10.1051/0004-6361:20010579en
local.identifier.pure3062ac0a-93d5-41cc-83c6-0f9783676036en
local.identifier.urlhttps://www.scopus.com/pages/publications/0035373080en
local.type.statusPublisheden

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