Discovery of PSR 1259-63 in VHE Gamma-Rays with H.E.S.S.

Details Discovery of PSR 1259-63 in VHE Gamma-Rays with H.E.S.S. Discovery of PSR 1259-63 in VHE Gamma-Rays with H.E.S.S.

Mar 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004atel..249....1b&link_type=abstract

The Astronomer's Telegram, #249

Astronomy and Astrophysics

Astronomy

1

Gamma Ray, >Gev, Request For Observations, Binaries, Pulsars

Scientific paper

We report detection of very-high-energy gamma-ray emission from the binary millisecond pulsar PSR 1259-63 (1236.72-day orbit) by the H.E.S.S. experiment above a threshold of about 200 GeV (in the observed zenith-angle range, 40o-45o) at the 5.9-sigma level, where previously upper limits were reported by the CANGAROO collaboration (Kawachi et al. 2004, Ap.J., in press).

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