{ "id": "2405.09612", "version": "v1", "published": "2024-05-15T18:00:01.000Z", "updated": "2024-05-15T18:00:01.000Z", "title": "Imprint of 'local opacity' effect in gamma-ray spectrum of blazar jet", "authors": [ "Sushmita Agarwal", "Amit Shukla", "Karl Mannheim", "Bhargav Vaidya", "Biswajit Banerjee" ], "comment": "10 pages, 3 figures, 1 table, accepted for publication in ApJL", "categories": [ "astro-ph.HE" ], "abstract": "Relativistic jets from accreting supermassive black holes at cosmological distances can be powerful emitters of $\\gamma$-rays. However, the precise mechanisms and locations responsible for the dissipation of energy within these jets, leading to observable $\\gamma$-ray radiation, remain elusive. We detect evidence for an intrinsic absorption feature in the $\\gamma$-ray spectrum at energies exceeding $10\\,$GeV, presumably due to the photon-photon pair production of $\\gamma$-rays with low ionization lines at the outer edge of Broad-line region (BLR), during the high-flux state of the flat-spectrum radio quasar PKS 1424$-$418. The feature can be discriminated from the turnover at higher energies resulting from $\\gamma$-ray absorption in the extragalactic background light. It is absent in the low-flux states supporting the interpretation that powerful dissipation events within or at the edge of the BLR evolve into fainter $\\gamma$-ray emitting zones outside the BLR, possibly associated with the moving VLBI radio knots. The inferred location of $\\gamma$-ray emission zone is consistent with the observed variability time scale of the brightest flare, provided that the flare is attributed to external Compton scattering with BLR photons.", "revisions": [ { "version": "v1", "updated": "2024-05-15T18:00:01.000Z" } ], "analyses": { "keywords": [ "gamma-ray spectrum", "local opacity", "blazar jet", "flat-spectrum radio quasar pks", "moving vlbi radio knots" ], "note": { "typesetting": "TeX", "pages": 10, "language": "en", "license": "arXiv", "status": "editable" } } }