2019/09/02 by Mabel Osorio, Osorio, Mabel, Sacahui, Rodrigo +6
Engineering · Physics and Astronomy · #Astrophysics and Cosmic Phenomena #FOS: Physical sciences #High Energy Astrophysical Phenomena (astro-ph.HE) #Neutrino Physics Research #Particle Accelerators and Free-Electron Lasers #Particle physics theoretical and experimental studies
paper · pdf · doi:10.48550/arxiv.1909.00897
openalex publication_date 2019/09/02 · openalex created_date 2022/07/28 · openalex updated_date 2026/07/28
The spectral energy distribution (SED) of blazars is generally understood\nthrough the standard one-zone synchrotron self-Compton (SSC) model, where a\nstrong correlation between X-ray and TeV gamma-ray fluxes is expected.\nRecently, for Mrk 421 the correlation was confirmed and interpreted within the\nSSC model arguing that a description of the correlation up to large flux values\nconsiderably restricts the value of the magnetic field under the assumption of\nan electron spectral index independent of the flux state. In this work, we\nextend the analysis done on Mrk 421 for other two high-energy peaked BL Lacs:\nMrk 501 and 1ES 1959+650.\n