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Masanori Ohno

Researcher at Hiroshima University

Publications -  264
Citations -  27442

Masanori Ohno is an academic researcher from Hiroshima University. The author has contributed to research in topics: Gamma-ray burst & Fermi Gamma-ray Space Telescope. The author has an hindex of 71, co-authored 258 publications receiving 25753 citations. Previous affiliations of Masanori Ohno include Eötvös Loránd University & Istituto Nazionale di Fisica Nucleare.

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The Large Area Telescope on the Fermi Gamma-ray Space Telescope Mission

W. B. Atwood, +292 more
TL;DR: The Large Area Telescope (Fermi/LAT) as mentioned in this paper is the primary instrument on the Fermi Gamma-ray Space Telescope, which is an imaging, wide field-of-view, high-energy gamma-ray telescope, covering the energy range from below 20 MeV to more than 300 GeV.
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Fermi Large Area Telescope Second Source Catalog

P. L. Nolan, +293 more
TL;DR: The second Fermi-LAT catalog (2FGL) as mentioned in this paper includes source location regions, defined in terms of elliptical fits to the 95% confidence regions and spectral fits in terms either power-law, exponentially cutoff power law, or log-normal forms.
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Fermi large area telescope first source catalog

A. A. Abdo, +288 more
TL;DR: The first Fermi-LAT catalog (1FGL) as mentioned in this paper contains 1451 sources detected and characterized in the 100 MeV to 100 GeV range, and the threshold likelihood Test Statistic is 25, corresponding to a significance of just over 4 sigma.
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The second fermi large area telescope catalog of gamma-ray pulsars

A. A. Abdo, +257 more
TL;DR: In this article, a catalog of gamma-ray pulsar detections using three years of data acquired by the Large Area Telescope (LAT) on the Fermi satellite is presented.
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Detection of the characteristic pion-decay signature in supernova remnants

Markus Ackermann, +200 more
- 15 Feb 2013 - 
TL;DR: The characteristic pion-decay feature is detected in the gamma-ray spectra of two SNRs, IC 443 and W44, with the Fermi Large Area Telescope, providing direct evidence that cosmic-ray protons are accelerated in SNRs.