Recent results from the CANGAROO 3.8 m telescope

Details Recent results from the CANGAROO 3.8 m telescope Recent results from the CANGAROO 3.8 m telescope

Jun 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aipc..515..192y&link_type=abstract

GeV-TeV GAMMA RAY ASTROPHYSICS WORKSHOP: Towards a Major Atmospheric Cherenkov Detector VI. AIP Conference Proceedings, Volume

Astronomy and Astrophysics

Astrophysics

1

Supernova Remnants, X-Ray Binaries, Pulsars, Gamma-Ray

Scientific paper

We observed the shell-type supernova remnant (SNR) RX J1713.7-3946 and the X-ray binaries Cen X-3 and Vela X-1 at TeV energies in 1998 using the CANGAROO 3.8 m telescope. Preliminary results of data analyses on these objects are summarized here. We also estimated a spectrum of the Vela pulsar region using 116 hr data taken by the 3.8 m telescope during 1994 and 1997. The two data sets having different mirror reflectivities give consistent results and the photon index of the best-fit power-law spectrum is -2.4+/-0.2. .

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