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000626005 1001_ $$0P:(DE-HGF)0$$aBatista, Pedro$$b0$$eCorresponding author$$gmale
000626005 245__ $$aA time sensitive modelling of the two extreme BL Lacertae objects 1ES 1218+304 and 1ES 0229+200$$f2019-11-01 - 2023-05-31
000626005 260__ $$bUniversität Potsdam$$c2024
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000626005 502__ $$aDissertation, Universität Potsdam, 2024$$bDissertation$$cUniversität Potsdam$$d2024$$o2024-12-03
000626005 520__ $$aIn this thesis, the broadband spectral energy distribution (SED) of the sources 1ES 1218+304 and 1ES 0229+200 is studied. 1ES 1218+304 and 1ES 0229+200 are two well-known extreme high-frequency-peaked BL Lac objects (EHBLs), a type of blazar. Blazars are in turn a type of active galactic nuclei (AGN) with the presence of a jet of relativistic charged particles where, by random chance, the jet points towards Earth. Data taken by the ultraviolet/optical telescope UVOT, and the X-ray telescope XRT, on board the Neils Gehrels Swift Observatory satellite, are used. The ultraviolet/optical and X-ray data are analysed together with gamma-ray data in the 30 MeV to 300 GeV range taken by the Fermi-LAT detector and in the 50 GeV to 30 TeV range, provided by the VERITAS Collaboration. The light curves of each energy band were built and analysed with a Bayesian blocks algorithm. The intrinsic spectral indices in the VHE range were found to be Γ
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000626005 650_7 $$2Other$$a520 Astronomie und zugeordnete Wissenschaften
000626005 650_7 $$2Other$$a530 Physik
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000626005 7001_ $$0P:(DE-HGF)0$$aElisa Pueschel, Dr.$$b1
000626005 7001_ $$0P:(DE-HGF)0$$aMartin Pohl, Prof. Dr.$$b2
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