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Gamma-ray bursts (GRBs) are cosmic events occurring at large distances beyond our galaxy. They provide a unique opportunity to study electromagnetic patterns not seen elsewhere. When the collimated GRB outflow interacts with the outer…

Gamma-Ray Bursts (GRBs) have been detected at GeV energies by EGRET and models predict emission at > 100 GeV. Milagro is a wide field (2 sr) high duty cycle (> 90 %) ground based water Cherenkov detector that records extensive air showers…

Astrophysics · Physics 2009-11-13 Pablo M. Saz Parkinson

We recalculate the diffuse flux of high energy neutrinos produced by Gamma Ray Bursts (GRB) in the relativistic fireball model. Although we confirm that the average single burst produces only ~10^{-2} high energy neutrino events in a…

Astrophysics · Physics 2009-10-31 F. Halzen , D. W. Hooper

Project GRAND presents the results of a search for coincident high-energy gamma ray events in the direction and at the time of nine Gamma Ray Bursts (GRBs) detected by BATSE. A gamma ray has a non-negligible hadron production cross section;…

Astrophysics · Physics 2007-05-23 T. F. Lin , J. Carpenter , S. Desch , J. Gress , J. Poirier , A. Roesch

Gamma-ray bursts (GRBs) are rare but powerful explosions displaying highly relativistic jets. It has been suggested that a significant fraction of the much more frequent core-collapse supernovae are accompanied by comparably energetic but…

Astrophysics · Physics 2007-05-23 Shin'ichiro Ando , John F. Beacom

Soft gamma-ray repeaters (SGR) are a class of high energy transients whose brief emissions are thought to arise from young and highly magnetized neutron stars. The exact cause for these outbursts and the nature of the energy loss remain…

Astrophysics · Physics 2009-10-31 D. A. Frail , S. R. Kulkarni , J. S. Bloom

Recent results link relativistic runaway electron avalanches (RREA) accelerated by the electric field in thunderclouds to high-energy atmospheric phenomena such as the Terrestrial Gamma-Ray Flashes (TGF). Research shows that the mere…

Atmospheric and Oceanic Physics · Physics 2023-07-12 Eduard Kim , Alexander Sedelnikov , Daria Zemlianskaya , Oraz Anuaruly , Egor Stadnichuk

Gamma-Ray Bursts (GRBs) directed at Earth from within a few kpc may have damaged the biosphere, primarily though changes in atmospheric chemistry which admit greatly increased Solar UV. However, GRBs are highly variable in spectrum and…

Astrophysics · Physics 2010-11-11 Larissa M. Ejzak , Adrian L. Melott , Mikhail V. Medvedev , Brian C. Thomas

The recent progress in studies of gamma-ray bursts, their afterglows, and host galaxies is discussed. The emphasis is given to high-energy phenomena associated with gamma-ray burst explosions: high-energy cosmic rays, neutrinos,…

Astrophysics · Physics 2007-05-23 K. A. Postnov

The Solar Tower Atmospheric Cherenkov Effect Experiment (STACEE) is an atmospheric Cherenkov telescope (ACT) that uses a large mirror array to achieve a relatively low energy threshold. For sources with Crab-like spectra, at high…

The aim of the present work is to study the potential short-term atmospheric and biospheric influence of Gamma Ray Bursts on the Earth. We focus in the ultraviolet flash at the planet's surface, which occurs as a result of the…

Earth and Planetary Astrophysics · Physics 2015-05-13 Osmel Martín , Douglas Galante , Rolando Cárdenas , J. E. Horvath

We have investigated TeV gamma-ray emissions from nearby X-ray selected BL Lac objects using the Utah Seven Telescope Array for more than two years. These objects can be considered as potential sources of TeV gamma rays with inverse compton…

Astrophysics · Physics 2012-08-27 The Utah Seven Telescope Array collaboration

The Telescope Array (TA) experiment is designed to observe cosmic-ray-induced air showers at extremely high energies. It is being deployed in a desert of Utah, USA; an array of 3 m^2 scintillation counters will be distributed over 760 km^…

Astrophysics · Physics 2007-05-23 K. kasahara

Gamma rays with energies greater than 7 TeV from the Crab pulsar/nebula have been observed at large zenith angles, using the Imaging Atmospheric Technique from Woomera, South Australia. CANGAROO data taken in 1992, 1993 and 1995 indicate…

We describe the MERger-event Gamma-Ray (MERGR) Telescope intended for deployment by ~2021. MERGR will cover from 20 keV to 2 MeV with a wide field of view (6 sr) using nineteen gamma-ray detectors arranged on a section of a sphere. The…

Instrumentation and Methods for Astrophysics · Physics 2017-11-13 L. J. Mitchell , J. E. Grove , B. F. Phlips , C. C. Cheung , M. Kerr , R. S. Woolf , M. S. Briggs , J. S. Perkins

The first limits on the prompt emission from the long gamma-ray burst (GRB) 130427A in the $>100\nobreakspace\rm{GeV}$ energy band are reported. GRB 130427A was the most powerful burst ever detected with a redshift $z\lesssim0.5$ and…

We show that with GLAST there will be the possibility to detect, within the UHECR skimming at atmosphere edges, the showers generated by very high energy upward and horizontal Tau. The effective area, thanks to the large area covered by the…

Astrophysics · Physics 2008-06-13 Daniele Fargion

The potentiality of a Giant Shower Array to low energy gamma rays from gamma ray bursts is discussed. Effective areas are calculated for different scenarios and the results are encouraging. If gamma ray bursts have a spectrum which…

Astrophysics · Physics 2007-05-23 C. O. Escobar , P. L. Da Silva , R. A. Vázquez

We present a comprehensive catalog and analysis of broad-band afterglow observations for 103 short-duration gamma-ray bursts (GRBs), comprised of all short GRBs from November 2004 to March 2015 with prompt follow-up observations in the…

High Energy Astrophysical Phenomena · Physics 2015-12-23 Wen-fai Fong , Edo Berger , Raffaella Margutti , B. Ashley Zauderer

In this paper, we present the results of Monte Carlo simulations of atmospheric showers induced by diffuse gamma rays as detected by the high-energy gamma ray astronomy (HEGRA) system of five imaging atmospheric Cerenkov telescopes (IACTs).…

Astrophysics · Physics 2008-11-26 A. Konopelko , F. Lucarelli , H. Lampeitl , W. Hofmann
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