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T. Richards, H. Fleischhack, H. Krawczynski, H. Prokoph, I. Telezhinsky, J. Dumm, J. Grube, J. H. Buckley, J. Holder, J. Millis, J. P. Finley, J. Quinn, J. S. Perkins, K. Berger, K. Byrum, K. Meagher, K. Ragan, L. Ciupik, L. C. Reyes, L. Fortson, M. Beilicke, M. Cerruti, M. Errando, M. J. Lang, M. Kertzman, M. P. Connolly, M. Pohl, M. Theiling, N. Galante, N. Park, P. Fortin, P. Kaaret, P. Majumdar, P. Moriarty, P. T. Reynolds, Q. Feng, R. A. Ong, R. Bird, R. Mukherjee, R. Welsing, S. Archambault, S. Federici, S. Griffin, S. McArthur, S. P. Wakely, S. T. Griffiths, S. Vincent, T. Arlen, T. Aune, T. B. Humensky, T. C. Weekes, V. Bugaev, V. V. Vassiliev, W. Benbow, W. Cui, X. Chen, Y. Khassen","submitted_at":"2013-12-23T16:31:57Z","abstract_excerpt":"The high-frequency-peaked BL Lacertae object 1ES 0229+200 is a relatively distant (z = 0.1396), hard-spectrum (Gamma ~ 2.5), very-high-energy-emitting (E > 100 GeV) gamma-ray blazar. 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