Simulating Cherenkov Telescope Array observation of RX J1713.7-3946

@article{Nakamori2015SimulatingCT,
  title={Simulating Cherenkov Telescope Array observation of RX J1713.7-3946},
  author={T. Nakamori and H. Katagiri and H. Sano and R. Yamazaki and Y. Ohira and A. Bamba and Y. Fukui and K. Mori and S. Lee and Y. Fujita and H. Tajima and T. Inoue and S. Gunji and Y. Hanabata and M. Hayashida and H. Kubo and J. Kushida and S. Inoue and K. Ioka and K. Kohri and K. Murase and S. Nagataki and T. Naito and A. Okumura and T. Saito and M. Sawada and T. Tanaka and Y. Terada and Y. Uchiyama and S. Yanagita and T. Yoshida and T. Yoshikoshi and For The Cta Consortium},
  journal={arXiv: High Energy Astrophysical Phenomena},
  year={2015}
}
We perform simulations of Cherenkov Telescope Array (CTA) observations of a young supernova remnant RX J1713.7-3946. This target is not only one of the brightest sources ever discovered in very high-energy gamma rays but also well observed in other wavebands. In X-rays, the emission is dominated by synchrotron radiation, which links directly to the existence of high-energy electrons. Radio observations of CO and HI gas have revealed a highly inhomogeneous medium surrounding the SNR, such as… Expand

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