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pro vyhledávání: '"Akbar, Sikandar"'
We conducted a multi-wavelength analysis of the blazar Mrk\,501, utilizing observations from \emph{Astro}Sat (SXT, LAXPC), \emph{Swift-UVOT}, and \emph{Fermi-LAT} during the period August 15, 2016 to March 27, 2022. The resulting multi-wavelength lig
Externí odkaz:
http://arxiv.org/abs/2411.00592
Publikováno v:
In Journal of High Energy Astrophysics November 2024 44:393-409