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Grube, J. H. Buckley, J. Holder, J. Millis, J. P. Finley, J. Quinn, J. Rousselle, J. Tyler, J. V Cardenzana, J. V. Tucci, K. Byrum, K. Meagher, K. Ragan, K. Shahinyan, L. Ciupik, L. Fortson, M. Buchovecky, M. Cerruti, M. Hutten, M. J. Lang, M. Kertzman, M. Krause, M. P. Connolly, M. Pohl, M. Santander, N. Hakansson, N. Kelley-Hoskins, N. Park, O. M. Weiner, P. Kaaret, P. Kar, P. Moriarty, P. T. Reynolds, Q. Feng, R. A. Ong, R. Bird, R. Mukherjee, S. Griffin, S. Kumar, S. McArthur, S. P. Wakely, T. B. Humensky, V. Bugaev, V. Pelassa, V. V. Vassiliev, W. Benbow, X. Chen","submitted_at":"2016-02-26T22:21:48Z","abstract_excerpt":"The Galactic Center Ridge has been observed extensively in the past by both GeV and TeV gamma-ray instruments revealing a wealth of structure, including a diffuse component as well as the point sources G0.9+0.1 (a composite supernova remnant) and Sgr A* (believed to be associated with the supermassive black hole located at the center of our Galaxy). 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