New Insights on Gamma Rays 2017
DOI: 10.5772/67176
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Gamma Rays from Space

Abstract: An overview of gamma rays from space is presented. We highlight the most powerful astrophysical explosions, known as gamma-ray bursts. The main features observed in detectors onboard satellites are indicated. In addition, we also highlight a chronological description of the efforts made to observe their high energy counterpart at ground level. Some candidates of the GeV counterpart of gamma-ray bursts, observed by Tupi telescopes, are also presented.

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Cited by 3 publications
(2 citation statements)
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“…Gamma rays were observed in 1900 by chemist Paul Villard [34]. Gamma rays (λ < 10 pm) are electromagnetic radiations with high energy (energy >100 keV) [35].…”
Section: Gamma Radiation Treatmentmentioning
confidence: 99%
“…Gamma rays were observed in 1900 by chemist Paul Villard [34]. Gamma rays (λ < 10 pm) are electromagnetic radiations with high energy (energy >100 keV) [35].…”
Section: Gamma Radiation Treatmentmentioning
confidence: 99%
“…Usually these effects result in an increase in the flux of secondary charged particles, such as electrons and muons produced by primary gamma rays in the atmosphere. Thus, more particles can reach the ground level and be registered by the detector [25,26,29] In this paper we report the results of a search for the particle excess above the background in coincidence with Fermi LAT detection of GRBs (ΣE γ > 100 MeV) in the period from from 8 June 2014 to 28 February 2017. In this period Fermi LAT detected 46 GRB events (https : //f ermi.gsf c.nasa.gov/ssc/observations/types/grbs/lat grbs/).…”
Section: Introductionmentioning
confidence: 99%