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This paper presents the results of a detailed X-ray timing and spectral analysis of Mrk 501 , which are based mainly on the Swift data obtained during 2021 February–2022 December. The source showed ...
are the HBLs Mrk 501 and PG 1553 + 113 objects. A preprint version of the article is available at ArXiv. Eur. Phys. J. C (2016) 76:127 DOI 10.1140/epjc/s10052-016-3975-2 Regular Article - Theoretical Physics ...
Abstract We compare the rise and decay time-scales of ∼200 long-term (∼weeks–months) GeV and R-band outbursts and ∼25 short-term (∼hour–day) GeV flares in a sample of 10 blazars from the Fermi-LAT ...
LSP No correlation 1ES1959+650 HSP No correlation 3C 66A HSP No correlation PKS 2155-304 HSP 4 ± 2 Mrk 421 HSP No correlation Mrk 501 HSP No correlation Sources Type Delay 3C 279 LSP 2 ± 1 3C 454.3 LSP ...
angles, the detection of MAGNs in the GeV band may be indicative of a different emission site or emission mechanism. An example is the RG Centaurus A, where the extended γ-ray component is most likely ...
-hadronic model, with both models fitting the data reasonably well. Aleksić et al. (2014a) found a cut-off in the GeV range of the high-energy SED of this source. This finding hints that the gamma-ray ...
-luminosity BL Lacs which are HSPs exhibit the synchrotron peak in the UV-soft X-ray band and the inverse Compton peak between the GeV and the TeV gamma-ray band (Padovani & Giommi 1995). In mid-luminosity ...
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