Observation of the galactic plane at energies above 0.6TeV

Details Observation of the galactic plane at energies above 0.6TeV Observation of the galactic plane at energies above 0.6TeV

Aug 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999icrc....3..390l&link_type=abstract

Proceedings of the 26th International Cosmic Ray Conference. August 17-25, 1999. Salt Lake City, Utah, USA. Under the auspices o

Physics

Scientific paper

In 1998 the Whipple Observatory 10 m telescope was used to observe the Galactic Plane at TeV energies. At this time, the telescope was equipped with a large (4:8o) field of view camera well suited to detect diffuse emission. We report here a preliminary analysis of these data. Assuming the TeV emission profile matches that found by EGRET above 1 GeV, we find an upper limit of 4:9 10,8s,1 cm,2 sr,1 average diffuse emission at galactic longitude 40o and energies above 0:6TeV. Further observations and analysis are in progress.

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