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تسجيل مستخدم جديدThe 2012 flare of PG 1553+113 seen with H.E.S.S. and Fermi-LAT
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Very high energy (VHE, $E>$100 GeV) $gamma$-ray flaring activity of the high-frequency peaked BL Lac object pg has been detected by the hess telescopes. The flux of the source increased by a factor of 3 during the nights of 2012 April 26 and 27 with respect to the archival measurements with hint of intra-night variability. No counterpart of this event has been detected in the fla data. This pattern is consistent with VHE $gamma$ ray flaring being caused by the injection of ultrarelativistic particles, emitting $gamma$ rays at the highest energies. The dataset offers a unique opportunity to constrain the redshift of this source at bestz using a novel method based on Bayesian statistics. The indication of intra-night variability is used to introduce a novel method to probe for a possible Lorentz Invariance Violation (LIV), and to set limits on the energy scale at which Quantum Gravity (QG) effects causing LIV may arise. For the subluminal case, the derived limits are $textrm{E}_{rm QG,1}>4.10times 10^{17}$ GeV and $textrm{E}_{rm QG,2}>2.10times 10^{10}$ GeV for linear and quadratic LIV effects, respectively.
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We investigate the axion like particle (ALP)-photon oscillation effect in the high energy $gamma$-ray spectra of PG 1553+113 and PKS 2155-304 measured by Fermi-LAT and H.E.S.S.. The choice of extragalactic background light (EBL) model, which induces
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ta were obtained with the KVA, REM, RossiXTE/ASM, AGILE and MAGIC telescopes. This is the first simultaneous broad-band (i.e., HE+VHE) gamma-ray observation of a blazar. The source spectral energy distribution derived combining these data shows the usual double-peak shape, and is interpreted in the framework of a synchrotron-self-Compton model.
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