{ "id": "astro-ph/0205441", "version": "v1", "published": "2002-05-24T21:27:40.000Z", "updated": "2002-05-24T21:27:40.000Z", "title": "Gravitational microlensing of gamma-ray blazars", "authors": [ "Diego F. Torres", "Gustavo E. Romero", "Ernesto F. Eiroa", "Joachim Wambsganss", "M. E. Pessah" ], "comment": "30 pages, 27 figures. Four figures are being submitted only as .gif files, and should be printed separately. The abstract below has been shortened from the actual version appearing in the paper", "journal": "Mon.Not.Roy.Astron.Soc.339:335-352,2003", "doi": "10.1046/j.1365-8711.2003.06219.x", "categories": [ "astro-ph", "gr-qc" ], "abstract": "We present a detailed study of the effects of gravitational microlensing on compact and distant $\\gamma$-ray blazars. These objects have $\\gamma$-ray emitting regions which are small enough as to be affected by microlensing effects produced by stars lying in intermediate galaxies. We analyze the temporal evolution of the gamma-ray magnification for sources moving in a caustic pattern field, where the combined effects of thousands of stars are taken into account using a numerical technique. We propose that some of the unidentified $\\gamma$-ray sources (particularly some of those lying at high galactic latitude whose gamma-ray statistical properties are very similar to detected $\\gamma$-ray blazars) are indeed the result of gravitational lensing magnification of background undetected Active Galactic Nuclei (AGNs).", "revisions": [ { "version": "v1", "updated": "2002-05-24T21:27:40.000Z" } ], "analyses": { "keywords": [ "gravitational microlensing", "gamma-ray blazars", "high galactic latitude", "background undetected active galactic nuclei", "ray sources" ], "tags": [ "journal article" ], "note": { "typesetting": "TeX", "pages": 30, "language": "en", "license": "arXiv", "status": "editable", "inspire": 587359 } } }