Preliminary Results on the Flux of TeV g-Rays from Crab System Obtained with the PACT at Pachmarhi

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Scientific paper

We have observed the Crab system (Nebula and Pulsar) and the
corresponding background regions during many clear nights in the years
1999-2002 ˇ using the atmospheric Cerenkov array at Pachmarhi,
PACT. Preliminary results indicate a steady emission of TeV γ
-rays from the Crab Nebula.

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