| Article ID | Journal | Published Year | Pages | File Type | 
|---|---|---|---|---|
| 1770922 | Astroparticle Physics | 2012 | 10 Pages | 
Abstract
												⺠A partly new analysis was applied to CANGAROO-III data. ⺠No evidence of TeV gamma-ray emissions were found from four blazars. ⺠Non-simultaneous multiwavelength SEDs of blazars were modeled with a leptonic scenario successfully. ⺠The magnetic field of H 2356-309 might be lower than so far reported values. ⺠We find a consistency with the blazar sequence in terms of the magnetic field and the size of blob.
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											Authors
												Y. Mizumura, J. Kushida, K. Nishijima, G.V. Bicknell, R.W. Clay, P.G. Edwards, S. Gunji, S. Hara, S. Hayashi, S. Kabuki, F. Kajino, A. Kawachi, T. Kifune, R. Kiuchi, K. Kodani, Y. Matsubara, T. Mizukami, Y. Mizumoto, T. Yoshikoshi, 
											