A new population of compton-thick AGNs identified using the spectral curvature above 10 keV.

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dc.contributor.authorKoss, M.
dc.contributor.authorBauer, Franz Erik
dc.contributor.authorRicci, Claudio
dc.contributor.authorTreister, Ezequiel
dc.contributor.authorAssef T., Roberto
dc.contributor.authorBalokovic, M.
dc.contributor.authorStern, Daniel.
dc.contributor.authorGandhi, P.
dc.contributor.authorLamperti, I.
dc.contributor.authorAlexander, D. M.
dc.date.accessioned2019-05-24T14:58:39Z
dc.date.available2019-05-24T14:58:39Z
dc.date.issued2016
dc.date.updated2019-05-17T16:00:57Z
dc.fuente.origenORCID
dc.identifier.doi10.3847/0004-637X/825/2/85
dc.identifier.issn1538-4357
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/22830
dc.identifier.urihttps://doi.org/10.3847/0004-637X/825/2/85
dc.issue.numeroNo. 2
dc.pagina.final18
dc.pagina.inicio1
dc.relation.isformatofThe Astrophysical Journal, vol. 825, no. 2 (July 2016), 18 p.
dc.revistaThe Astrophysical Journales_ES
dc.rightsacceso abierto
dc.subjectGalaxieses_ES
dc.subjectActive - galaxieses_ES
dc.subjectSeyfert - X-rayses_ES
dc.subject.ddc520
dc.subject.deweyAstronomíaes_ES
dc.titleA new population of compton-thick AGNs identified using the spectral curvature above 10 keV.es_ES
dc.typeartículo
dc.volumenVol. 825
sipa.codpersvinculados1007961
sipa.codpersvinculados1015217
sipa.codpersvinculados1031846
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