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Gamma-gamma absorption in the broad line region radiation fields of gamma-ray blazars. ERRATUM. (2016, ApJ, 821, 102)

dc.contributor.authorBöttcher, Markus
dc.contributor.authorEls, Paul
dc.contributor.researchID22934537 - Els, Paul Lodewyk
dc.contributor.researchID24420530 - Böttcher, Markus
dc.date.accessioned2019-02-04T11:21:57Z
dc.date.available2019-02-04T11:21:57Z
dc.date.issued2018
dc.description.abstractIn the published article, our code to evaluate the γγ opacity due to the BLR radiation field contained a numerical error, due to which all opacities are a factor of 2π too low. The corrected Figures 2-4 are shown below. The conclusions of the paper do not change qualitatively, but the constraints on the location of the γ-ray emission region become tighter. In particular, in the case of 3C279, VHE photons beyond ~300 GeV, must be emitted significantly beyond the BLR, if produced by Compton scattering of BLR photonsen_US
dc.identifier.citationBöttcher, M. & Els, P. 2018. Gamma-gamma absorption in the broad line region radiation fields of gamma-ray blazars. ERRATUM. (2016, ApJ, 821, 102). Astrophysical journal, 869(1): Article no 87. [https://doi.org/10.3847/1538-4357/aaf04c]en_US
dc.identifier.issn0004-637X
dc.identifier.issn1538-4357 (Online)
dc.identifier.urihttp://hdl.handle.net/10394/31787
dc.identifier.urihttps://iopscience.iop.org/article/10.3847/1538-4357/aaf04c/pdf
dc.identifier.urihttps://doi.org/10.3847/1538-4357/aaf04c
dc.language.isoenen_US
dc.publisherIOP Publishingen_US
dc.titleGamma-gamma absorption in the broad line region radiation fields of gamma-ray blazars. ERRATUM. (2016, ApJ, 821, 102)en_US
dc.typeArticleen_US

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