학술논문

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

Document Type

Working Paper

Author

Kildea, J.; Zweerink, J.; Ball, J.; Carson, J. E.; Covault, C. E.; Driscoll, D. D.; Fortin, P.; Gingrich, D. M.; Hanna, D. S.; Jarvis, A.; Lindner, T.; Mueller, C.; Mukherjee, R.; Ong, R. A.; Ragan, K.; Williams, D. A.

Source

Subject

Astrophysics

Language

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.
Comment: 4 pages, 1 figure, ICRC 2007 conference proceedings

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Open Access (Arxiv) Find it@PNU

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