dc.creatorLira Teillery, Paulina
dc.creatorBotti, Ismael
dc.creatorKaspi, Shai
dc.creatorNetzer, Hagai
dc.date.accessioned2018-07-20T17:20:41Z
dc.date.available2018-07-20T17:20:41Z
dc.date.created2018-07-20T17:20:41Z
dc.date.issued2018
dc.identifierFront. Astron. Space Sci. 4: 71
dc.identifier10.3389/fspas.2017.00071
dc.identifierhttps://repositorio.uchile.cl/handle/2250/150097
dc.description.abstractWe present Reverberation Mapping results after monitoring a sample of 17 high-z, high-luminosity quasars for more than 10 years using photometric and spectroscopic capabilities. Continuum and line emission flux variability is observed in all quasars. Using cross-correlation analysis we successfully determine lags between the variations in the continuum and broad emission lines for several sources. Here we present a highlight of our results and the determined radius-luminosity relations for Ly alpha and CIV.
dc.languageen
dc.publisherFrontiers media SA
dc.rightshttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/
dc.rightsAttribution-NonCommercial-NoDerivs 3.0 Chile
dc.sourceFrontiers in Astronomy and Space Sciences
dc.subjectQuasars
dc.subjectBlack holes
dc.subjectReverberation mapping
dc.subjectBroad line region
dc.subjectAGN
dc.titleReverberation mapping of High - z, High - luminosity quasars
dc.typeArtículo de revista


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