1. CANGAROO-III observation of TeV gamma rays from the unidentified gamma-ray source HESS J1614-518
- Author
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Mizukami, T., Kubo, H., Yoshida, T., Nakamori, T., Enomoto, R., Tanimori, T., Akimoto, M., Bicknell, G. V., Clay, R. W., Edwards, P. G., Gunji, S., Hara, S., Hara, T., Hayashi, S., Ishioka, H., Kabuki, S., Kajino, F., Katagiri, H., Kawachi, A., Kifune, T., Kiuchi, R., Kunisawa, T., Kushida, J., Matoba, T., Matsubara, Y., Matsuzawa, I., Mizumura, Y., Mizumoto, Y., Mori, M., Muraishi, H., Naito, T., Nakayama, K., Nishijima, K., Ohishi, M., Otake, Y., Ryoki, S., Saito, K., Sakamoto, Y., Stamatescu, V., Suzuki, T., Swaby, D. L., Thornton, G., Tokanai, F., Toyota, Y., Tsuchiya, K., Yanagita, S., Yokoe, Y., Yoshikoshi, T., and Yukawa, Y.
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Astrophysics - High Energy Astrophysical Phenomena - Abstract
We report the detection, with the CANGAROO-III imaging atmospheric Cherenkov telescope array, of a very high energy gamma-ray signal from the unidentified gamma-ray source HESS J1614-518, which was discovered in the H.E.S.S. Galactic plane survey. Diffuse gamma-ray emission was detected above 760 GeV at the 8.9 sigma level during an effective exposure of 54 hr from 2008 May to August. The spectrum can be represented by a power-law: 8.2+-2.2_{stat}+-2.5_{sys}x10^{-12}x (E/1TeV)^{-Gamma} cm^{-2} s^{-1} TeV^{-1} with a photon index Gamma of 2.4+-0.3_{stat}+-0.2_{sys}, which is compatible with that of the H.E.S.S. observations. By combining our result with multi-wavelength data, we discuss the possible counterparts for HESS J1614-518 and consider radiation mechanisms based on hadronic and leptonic processes for a supernova remnant, stellar winds from massive stars, and a pulsar wind nebula. Although a leptonic origin from a pulsar wind nebula driven by an unknown pulsar remains possible, hadronic-origin emission from an unknown supernova remnant is preferred., Comment: 9 pages, 7 figures, accepted for publication in ApJ
- Published
- 2011
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