Evidence of TeV gamma-ray emission from the nearby starburst galaxy NGC 253

C. Itoh, R. Enomoto*, S. Yanagita, T. Yoshida, T. Tanimori, K. Okumura, A. Asahara, G. V. Bicknell, R. W. Clay, P. G. Edwards, S. Gunji, S. Hara, T. Hara, T. Hattori, Shin Hayashi, Sei Hayashi, S. Kabuki, F. Kajino, H. Katagiri, A. KawachiT. Kifune, H. Kubo, J. Kushida, Y. Matsubara, Y. Mizumoto, M. Mori, H. Moro, H. Muraishi, Y. Muraki, T. Naito, T. Nakase, D. Nishida, K. Nishijima, M. Ohishi, J. R. Patterson, R. J. Protheroe, K. Sakurazawa, D. L. Swaby, F. Tokanai, K. Tsuchiya, H. Tsunoo, T. Uchida, A. Watanabe, S. Watanabe, T. Yoshikoshi

*Corresponding author for this work

    Research output: Contribution to journalArticlepeer-review

    25 Citations (Scopus)

    Abstract

    TeV gamma-rays were recently detected from the nearby normal spiral galaxy NGC 253 (Itoh et al. 2002). Observations to detect the Cherenkov light images initiated by gamma-rays from the direction of NGC 253 were carried out in 2000 and 2001 over a total period of ∼150 hours. The orientation of images in gamma-ray-like events is not consistent with emission from a point source, and the emission region corresponds to a size greater than 10 kpc in radius. Here, detailed descriptions of the analysis procedures and techniques are given.

    Original languageEnglish
    Pages (from-to)443-455
    Number of pages13
    JournalAstronomy and Astrophysics
    Volume402
    Issue number2
    DOIs
    Publication statusPublished - 2003

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