Observation of gamma-rays greater than 10 TeV from Markarian 421
Abstract
We have observed Markarian 421 in January and March 2001 with the CANGAROO-II imaging Cherenkov telescope during an extraordinarily high state at TeV energies. From 14 hours observations at very large zenith angles, , a signal of 298 52 gamma-ray--like events (5.7 ) was detected at TeV, where a higher sensitivity is achieved than those of usual observations near the zenith, owing to a greatly increased collecting area. Under the assumption of an intrinsic power-law spectrum, we derived a differential energy spectrum dN/dE = (3.3 \pm 0.9_{stat.} \pm 0.3_{syst.})\times10^{-13} (E/10 {Te V})^{-(4.0 ^{+0.9}_{-0.6}_{stat.} \pm 0.3_{syst.})} ph./cm/sec/TeV, which is steeper than those previously measured around 1 TeV, and supports the evidence for a cutoff in the spectrum of Markarian 421. However, the 4 excess at energies greater than 20 TeV in our data favors a cutoff energy of 8 TeV, at the upper end of the range previously reported from measurements at TeV energies.
Keywords
Cite
@article{arxiv.astro-ph/0209487,
title = {Observation of gamma-rays greater than 10 TeV from Markarian 421},
author = {K. Okumura and A. Asahara and G. V. Bicknell and P. G. Edwards and R. Enomoto and S. Gunji and S. Hara and T. Hara and S. Hayashi and C. Itoh and S. Kabuki and F. Kajino and H. Katagiri and J. Kataoka and A. Kawachi and T. Kifune and H. Kubo and J. Kushida and S. Maeda and A. Maeshiro and Y. Matsubara and Y. Mizumoto and M. Mori and M. Moriya and H. Muraishi and Y. Muraki and T. Naito and T. Nakase and K. Nishijima and M. Ohishi and J. R. Patterson and K. Sakurazawa and R. Suzuki and D. L. Swaby and K. Takano and T. Takano and T. Tanimori and F. Tokanai and K. Tsuchiya and H. Tsunoo and K. Uruma and A. Watanabe and S. Yanagita and T. Yoshida and T. Yoshikoshi},
journal= {arXiv preprint arXiv:astro-ph/0209487},
year = {2009}
}
Comments
13 pages, 4 figures, to appear in Astrophisical Journal Letters