The x-ray luminous galaxy cluster population at 0.9 < z ≲ 1.6 as revealed by the XMM-Newton Distant Cluster Project

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dc.contributor.authorFassbender, R.
dc.contributor.authorQuintana Godoy, Hernán
dc.date.accessioned2016-05-10T18:15:05Z
dc.date.available2016-05-10T18:15:05Z
dc.date.issued2011
dc.identifier.doi10.1051/0004-6361/201015204
dc.identifier.issn1367-2630
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/13597
dc.identifier.urihttps://doi.org/10.1088/1367-2630/13/12/125014
dc.identifier.wosidWOS:000287484100093
dc.language.isoen
dc.nota.accesocontenido completo
dc.pagina.final53
dc.pagina.inicio1
dc.relation.isformatofNew Journal of Physics Vol. 13, Art. 125014.
dc.revistaNew Journal of Physicses_ES
dc.rightsacceso abierto
dc.subject.ddc520
dc.subject.deweyAstronomíaes_ES
dc.subject.otherCúmulos de galaxiases_ES
dc.subject.otherAstronomía de rayos Xes_ES
dc.subject.otherAstronomía infrarroja . Observacioneses_ES
dc.subject.otherAstrofísicaes_ES
dc.titleThe x-ray luminous galaxy cluster population at 0.9 < z ≲ 1.6 as revealed by the XMM-Newton Distant Cluster Project
dc.typeartículo
dc.volumenVol. 13
sipa.codpersvinculados98960
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