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Fortson, M. Buchovecky, M. Cerruti, M. Errando, M. Hutten, M. J. Lang, M. Kertzman, M. Krause, M. P. Connolly, M. Pohl, M. Santander, N. Kelley-Hoskins, N. Park, P. Kaaret, P. Kar, P. Moriarty, P. Slane, P. T. Reynolds, P. Wilcox, Q. Feng, R. A. Ong, R. Bird, R. Mukherjee, S. Griffin, S. Kumar, S. McArthur, S. O'Brien, S. P. Wakely, S. Trepanier, T. Weisgarber, V. Bugaev, VERITAS Collaboration: S. Archambault, V. V. Dwarkadas, W. Benbow, W. Cui","submitted_at":"2017-01-24T06:04:42Z","abstract_excerpt":"High-energy gamma-ray emission from supernova remnants (SNRs) has provided a unique perspective for studies of Galactic cosmic-ray acceleration. Tycho's SNR is a particularly good target because it is a young, type Ia SNR that is well-studied over a wide range of energies and located in a relatively clean environment. 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