activity
19962021
most citedDirect Measurement of the Cosmic-Ray Proton Spectrum from 50 GeV to 10 TeV with the Calorimetric Electron Telescope on the International Space Station

180 citations · 1.6k across the 55 of their papers we have counts for

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astro-ph2008★ 4 cited

Recent Topics on Very High Energy Gamma-ray Astronomy

Masaki Mori

With the advent of imaging atmospheric Cherenkov telescopes in late 1980's, ground-based observation of TeV gamma-rays came into reality after struggling trials by pioneers for twe…

astro-ph2007

MITSuME--Multicolor Imaging Telescopes for Survey and Monstrous Explosions

T. Kotani, N. Kawai, K. Yanagisawa +25

Development of MITSuME is reported. Two 50-cm optical telescopes have been built at Akeno in Yamanashi prefecture and at Okayama Astrophysical Observatory (OAO) in Okayama prefectu…

astro-ph2005

The search for optical emission on and before the GRB trigger with the WIDGET telescope

T. Tamagawa, F. Usui, Y. Urata +11

WIDGET is a robotic telescope for monitoring the HETE-2 field-of-view to detect Gamma-ray Burst optical flashes or possible optical precursors. The system has 62degx62deg wide fiel…

astro-ph2004★ 7 cited

Gamma-ray Spectra due to Cosmic-ray Interactions with Dense Gas Clouds

Michiko Ohishi, Masaki Mori, Mark Walker

Gamma-ray spectra from cosmic-ray proton and electron interactions with dense gas clouds have been calculated using a Monte Carlo event simulation code, GEANT4. Such clouds are pos…

astro-ph2002★ 11 cited

Dense gas clouds and the Unidentified EGRET sources

Mark Walker, Masaki Mori, Michiko Ohishi

Cold, dense gas clouds have been proposed as a major component of the Galactic dark matter; such clouds can be revealed by the gamma-ray emission which arises from cosmic-rays inte…

astro-ph2002★ 27 cited

Development of an atmospheric Cherenkov imaging camera for the CANGAROO-III experiment

S. Kabuki, K. Tsuchiya, K. Okumura +10

A Cherenkov imaging camera for the CANGAROO-III experiment has been developed for observations of gamma-ray induced air-showers at energies from 10 to 10 eV. The came…