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Evidence for a Point Source of High Energy Cosmic Gamma Rays

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TLDR
In this paper, high energy cosmic gamma radiation detection from point source in Sagittarius, using balloon mounted spark chamber with Cerenkov telescope, was performed using a single point source.
Abstract
High energy cosmic gamma radiation detection from point source in Sagittarius, using balloon mounted spark chamber with Cerenkov telescope

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Journal ArticleDOI

High-energy gamma-ray astronomy.

TL;DR: Gamma-ray astronomy above 10 MeV is difficult from the experimental point of view, but promising data are beginning to appear, as this survey progress report shows.
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The neutral-pion decay and the gamma radiation from our galaxy

TL;DR: Neutral pion decay and galactic gamma radiation from demodulated cosmic ray spectrum, discussing neutral pion meson production was discussed in this article, where the authors also discussed the role of neutral pions in meson creation.
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Galactic gamma-radiation between 200 MeV and 10 GeV.

TL;DR: This experiment was undertaken to study the high energy part of the spectrum between 200 MeV and 10 GeV, using balloon-borne detectors, and concluded that γ-ray emission from the Galaxy is predominantly diffuse line flux from the galactic disk.
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Detection of 10–100 MeV γ-Rays from the Crab Nebula Pulsar NP 0532

TL;DR: In this paper, the energy spectrum of the main pulse from 1 keV to 100 MeV can be fitted by a single power law of index (−0.9) for the γ-ray emission from NP 532.
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Physical Sciences: Two New Point Sources of High Energy Cosmic Gamma Rays

TL;DR: In this paper, the authors reported the detection of a high energy γ-ray source from neutral pion decay, inverse Compton collisions and bremsstrahlung2-6.
References
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Journal ArticleDOI

Observation of high-energy cosmic gamma rays.

TL;DR: High energy cosmic gamma radiation coincident with galactic plane observed by detector on OSO 3 was detected in this article, where the galactic plane was assumed to be a Gaussian cloud.
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Spark chamber for gamma-ray astronomy

TL;DR: In this article, a spark chamber system is described which is designed to detect γ rays in the cosmic radiation on high altitude balloon flights, using a magnetometer direction monitor locates the γ ray direction to ±3° in right ascension and declination.
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