S. Ogio

Very high energy gamma rays from PSR 1706-44

We have obtained evidence of gamma-ray emission above 1 TeV from PSR1706-44, using a ground-based telescope of the atmospheric \v{C}erenkov imaging type located near Woomera, South Australia. This object, a

OBSERVATION OF THE 7 TEV GAMMA RAYS FROM THE CRAB USING THE LARGE ZENITH ANGLE AIR CERENKOV IMAGING TECHNIQUE

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Long-lived solar neutron emission in comparison with electron-produced radiation in the 2005 September 7 solar flare

-ray source discovered by the COS B satellite (2CG342-02), was identified with the radio pulsar through the discovery of a 102 ms pulsed signal with the EGRET instrument of the Compton Gamma Ray Observatory. The flux of the present observation above a threshold of 1 TeV is

Calibration of photomultiplier tubes for the fluorescence detector of telescope array experiment using a Rayleigh scattered laser beam

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An Event Reconstruction Method for the Telescope Array Fluorescence Detectors

1

Measurement of ultra-high energy cosmic rays by telescope array (ta)

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Central Laser Facility Analysis at The Telescope Array Experiment

10

The telescope array low energy extension (TALE)

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Search for isotropic microwave radiation from electron beam in the atmosphere

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The Telescope Array experiment

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