Revealing a population of heavily obscured active galactic nuclei at z approximate to 0.5-1 in the chandra deep field-south

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dc.contributor.authorLuo, B.
dc.contributor.authorBauer, Franz Erik
dc.date.accessioned2016-05-10T18:02:18Z
dc.date.available2016-05-10T18:02:18Z
dc.date.issued2011
dc.identifier.issn0004-637X
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/12192
dc.language.isoen
dc.relation.isformatofAstrophysical Journal No. 1 (740), Art. 37.
dc.revistaAstrophysical Journales_ES
dc.subject.ddc520
dc.subject.deweyAstronomíaes_ES
dc.subject.otherAstronomía - Observacioneses_ES
dc.subject.otherAstronomía de rayos Xes_ES
dc.subject.otherAstrofísicaes_ES
dc.titleRevealing a population of heavily obscured active galactic nuclei at z approximate to 0.5-1 in the chandra deep field-southes_ES
dc.typeartículo
sipa.codpersvinculados1007961
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