TeV Gamma-Ray Spectra Unfolded for IR Absorption for a Sample of Low and High Red-Shifted AGN

Simple item page
dc.creatorKonopelko, A.
dc.creatorMastichiadis, A.
dc.creatorStecker, F. W.
dc.date2005-07-20
dc.date.accessioned2026-07-07T02:18:18Z
dc.date.available2026-07-07T02:18:18Z
dc.descriptionThe H.E.S.S. collaboration recently performed the accurate measurements of the gamma-ray spectra above 200 GeV for two BL Lac-type AGN in the Southern sky: PKS 2155-304 and PKS 2005-489. The TeV spectrum of the BL Lac object 1ES 2344+514 has also been recently measured by the Whipple collaboration. Using the results of phenomenological calculations of the SED of the EBL we have extracted the intrinsic gamma-ray spectra of these blazars. Consequently we have shown that these spectra can be fitted well by means of a synchrotron self Compton model.
dc.description4 pages, 1 figure, Proc. of 29th ICRC, Pune, India, 2005
dc.identifierhttps://arxiv.org/abs/astro-ph/0507479
dc.identifierhttp://arxiv.org/abs/astro-ph/0507479
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/9437
dc.subjectAstrophysics
dc.titleTeV Gamma-Ray Spectra Unfolded for IR Absorption for a Sample of Low and High Red-Shifted AGN
dc.typetext

Files

Collections

arXiv