The unresolved hard X-ray background: the missing source population implied by the Chandra and XMM Newton deep fields

dc.creatorBauer, Franz Erik
dc.date.accessioned2017-04-10T20:44:30Z
dc.date.available2017-04-10T20:44:30Z
dc.date.created2017-04-10T20:44:30Z
dc.date.issued2005
dc.identifier0035-8711
dc.identifierhttps://repositorio.uc.cl/handle/11534/18011
dc.identifierhttps://doi.org/10.1111/j.1365-2966.2005.08731.x
dc.identifier10.1086/496918
dc.languageen
dc.relationMonthly Notices of the Royal Astronomical Society. Vol. 357, no. 4 (2005), p. [1281]-1287
dc.titleThe unresolved hard X-ray background: the missing source population implied by the Chandra and XMM Newton deep fields
dc.typeArtículo


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