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20 April 2024

» arxiv » 0710.4623

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Observations of the Pulsar PSR B1951+32 with the Solar Tower Atmospheric Cherenkov Effect Experiment
J. Kildea ; J. Zweerink ; J. Ball ; J.E. Carson ; C. E. Covault ; D.D. Driscoll ; P. Fortin ; D. M. Gingrich ; D. S. Hanna ; A. Jarvis ; T. Lindner ; C. Mueller ; R. Mukherjee ; R. A. Ong ; K. Ragan ; D. A. William ;
Date:	25 Oct 2007
Abstract:	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 Experiment (STACEE). STACEE is an atmospheric Cherenkov detector, in Albuquerque, New Mexico, that detects cosmic gamma rays using the shower-front-sampling technique. STACEE’s sensitivity to astrophysical sources at energies around 100 GeV allows it to investigate emission from gamma-ray pulsars with expected pulsed emission cutoffs below 100 GeV. We discuss the observations and analysis of STACEE’s PSR 1951+32 data, accumulated during the 2005 and 2006 observing seasons.
Source:	arXiv, 0710.4623
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