activity
19962008
most citedStudy of highly-excited string states at the Large Hadron Collider

32 citations · 82 across the 11 of their papers we have counts for

collaborators
Showing 2007Show all

6 papers · 1 filter

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…

hep-ph20075 cited

Microcanonical treatment of black hole decay at the Large Hadron Collider

Douglas M. Gingrich, Kevin Martell

This study of corrections to the canonical picture of black hole decay in large extra dimensions examines the effects of back-reaction corrected and microcanonical emission at the…

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…