PULSED VERY HIGH ENERGY γ-RAY EMISSION CONSTRAINTS FOR PSR B1951+32 FROM STACEE OBSERVATIONS

Autor:	John Kildea, R. A. Ong, Corbin Covault, K. Ragan, Douglas Gingrich, D. S. Hanna, David A. Williams, J. Carson, Reshmi Mukherjee, P. Fortin, Jeffrey Zweerink, C. Mueller, D. D. Driscoll, T. Lindner, A. Jarvis, J. Ball
Rok vydání:	2009
Předmět:	Physics Range (particle radiation) Photon Astrophysics::High Energy Astrophysical Phenomena Gamma ray Astronomy Astronomy and Astrophysics Astrophysics STACEE law.invention Telescope Pulsar Space and Planetary Science law Cherenkov radiation Energy (signal processing)
Zdroj:	The Astrophysical Journal. 693:1128-1132
ISSN:	1538-4357 0004-637X
DOI:	10.1088/0004-637x/693/2/1128
Popis:	The Solar Tower Atmospheric Cherenkov Effect Experiment (STACEE) is a ground-based telescope that uses the wave-front-sampling technique to detect very high energy (VHE) gamma rays. STACEE's sensitivity in the energy range near 100 GeV permits useful observations of pulsars with the potential to discriminate between various proposed mechanisms for pulsed gamma-ray emission. Based on the 11.3 hr of data taken during the 2005 and 2006 observing seasons, we derive an upper limit on the pulsed gamma-ray emission from PSR B1951+32 of
Databáze:	OpenAIRE
Externí odkaz:	https://explore.openaire.eu/search/publication?articleId=doi_________::e707cac6df44348b472e3a794f7b34a1 https://doi.org/10.1088/0004-637x/693/2/1128 Zobrazit plný text záznamu