Search for 50 GeV emission from pulsar PSR B1951+32

Details Search for 50 GeV emission from pulsar PSR B1951+32 Search for 50 GeV emission from pulsar PSR B1951+32

Apr 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aps..aprn17031s&link_type=abstract

American Physical Society, April Meeting, Jointly Sponsored with the High Energy Astrophysics Division (HEAD) of the American As

Astronomy and Astrophysics

Astrophysics

Scientific paper

The CELESTE gamma ray telescope collects atmospheric Cherenkov light using 53 heliostats of the former solar facility "Themis", in the French Pyrenees. For pulsar searches the telescope is sensitive down to 20 GeV. We present results of observations of PSR B1951+32 and discuss whether gamma rays from this source come from the polar gap or from the outer gap.

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