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astro-ph2007

Observations of the Pulsar PSR B1951+32 with the Solar Tower Atmospheric Cherenkov Effect Experiment

J. Kildea, J. Zweerink, J. Ball +13

We present the analysis and results of 12.5 hours of high-energy gamma-ray observations of the EGRET-detected pulsar PSR B1951+32 using the Solar Tower Atmospheric Cherenkov Effect…

astro-ph20071 cited

STACEE Observations of 1ES 1218+304

STACEE Collaboration, R. Mukherjee, N. Akhter +15

We present the analysis and results of recent high-energy gamma-ray observations of the high energy-peaked BL Lac (HBL) object 1ES 1218+304 with the Solar Tower Atmospheric Cherenk…

astro-ph2007

Gamma-Ray Burst Follow-up Observations with STACEE During 2003-2007

STACEE Collaboration, A. Jarvis, J. Ball +14

The Solar Tower Atmospheric Cherenkov Effect Experiment (STACEE) is an atmospheric Cherenkov telescope (ACT) that uses a large mirror array to achieve a relatively low energy thres…

astro-ph20071 cited

Search for Dark Matter Annihilation in Draco with STACEE

STACEE Collaboration, D. D. Driscoll, J. Ball +14

For some time, the Draco dwarf spheroidal galaxy has garnered interest as a possible source for the indirect detection of dark matter. Its large mass-to-light ratio and relative pr…

astro-ph20073 cited

Very high energy observations of the BL Lac objects 3C 66A and OJ 287

T. Lindner, D. S. Hanna, J. Kildea +15

Using the Solar Tower Atmospheric Cherenkov Effect Experiment (STACEE), we have observed the BL Lac objects 3C 66A and OJ 287. These are members of the class of low-frequency-peake…

astro-ph200724 cited

Very High Energy Observations of Gamma-Ray Burst Locations with the Whipple Telescope

D. Horan, R. W. Atkins, H. M. Badran +56

Gamma-ray burst (GRB) observations at very high energies (VHE, E > 100 GeV) can impose tight constraints on some GRB emission models. Many GRB afterglow models predict a VHE compon…