166siThe mechanisms producing fast variability of the γ-ray emission in active galactic nuclei (AGNs) are under debate. The MAGIC telescopes detected a fast, very-high-energy (VHE, E > 100 GeV) γ-ray flare from BL Lacertae on 2015 June 15. The flare had a maximum flux of (1.5 ± 0.3) × 10^-10 photons cm-2 s-1 and halving time of 26 ± 8 min. The MAGIC observations were triggered by a high state in the optical and high-energy (HE, E > 100 MeV) γ-ray bands. In this paper we present the MAGIC VHE γ-ray data together with multi-wavelength data from radio, optical, X-rays, and HE γ rays from 2015 May 1 to July 31. Well-sampled multi-wavelength data allow us to study the variability in detail and compare it to the other epochs when fast, VHE γ-ray ...
175siAims. In the presence of a sufficient amount of target material, γ-rays can be used as a tracer...
The flat spectrum radio quasar (FSRQ) PKS 1510-089 is known for its complex multiwavelength behaviou...
153siSNR G24.7+0.6 is a 9.5 kyrs radio and γ-ray supernova remnant evolving in a dense medium. In th...
The mechanisms producing fast variability of the γ-ray emission in active galactic nuclei (AGNs) are...
164si1ES 1959+650 is a bright TeV high-frequency-peaked BL Lac object exhibiting interesting feature...
The mechanisms producing fast variability of the gamma-ray emission in active galactic nuclei (AGNs)...
149A neutrino with energy ˜290 TeV, IceCube-170922A, was detected in coincidence with the BL Lac obj...
177siExtreme high-frequency-peaked BL Lac objects (EHBLs) are blazars that exhibit extremely energet...
The flat spectrum radio quasar (FSRQ) PKS 1510-089 is known for its complex multiwavelength behavior...
We present optical, X-ray, high-energy (30 GeV) and very high energy (100 GeV; VHE) observations of ...
146siThe microquasar V404 Cygni underwent a series of outbursts in 2015, June 15–31, during which it...
© 2018. The American Astronomical Society. All rights reserved.. We report the AGILE detection and t...
154siWe report on the detection of flaring activity from the Fanaroff-Riley I radio galaxy NGC 1275 ...
The flat spectrum radio quasar (FSRQ) PKS 1510−089 is known for its complex multiwavelength behaviou...
164siThe Major Atmospheric Gamma-ray Imaging Cherenkov (MAGIC) telescopes observed S2 0109+22 in 201...
175siAims. In the presence of a sufficient amount of target material, γ-rays can be used as a tracer...
The flat spectrum radio quasar (FSRQ) PKS 1510-089 is known for its complex multiwavelength behaviou...
153siSNR G24.7+0.6 is a 9.5 kyrs radio and γ-ray supernova remnant evolving in a dense medium. In th...
The mechanisms producing fast variability of the γ-ray emission in active galactic nuclei (AGNs) are...
164si1ES 1959+650 is a bright TeV high-frequency-peaked BL Lac object exhibiting interesting feature...
The mechanisms producing fast variability of the gamma-ray emission in active galactic nuclei (AGNs)...
149A neutrino with energy ˜290 TeV, IceCube-170922A, was detected in coincidence with the BL Lac obj...
177siExtreme high-frequency-peaked BL Lac objects (EHBLs) are blazars that exhibit extremely energet...
The flat spectrum radio quasar (FSRQ) PKS 1510-089 is known for its complex multiwavelength behavior...
We present optical, X-ray, high-energy (30 GeV) and very high energy (100 GeV; VHE) observations of ...
146siThe microquasar V404 Cygni underwent a series of outbursts in 2015, June 15–31, during which it...
© 2018. The American Astronomical Society. All rights reserved.. We report the AGILE detection and t...
154siWe report on the detection of flaring activity from the Fanaroff-Riley I radio galaxy NGC 1275 ...
The flat spectrum radio quasar (FSRQ) PKS 1510−089 is known for its complex multiwavelength behaviou...
164siThe Major Atmospheric Gamma-ray Imaging Cherenkov (MAGIC) telescopes observed S2 0109+22 in 201...
175siAims. In the presence of a sufficient amount of target material, γ-rays can be used as a tracer...
The flat spectrum radio quasar (FSRQ) PKS 1510-089 is known for its complex multiwavelength behaviou...
153siSNR G24.7+0.6 is a 9.5 kyrs radio and γ-ray supernova remnant evolving in a dense medium. In th...