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Christy, B. Eberhardt, B. Eichmann, B. Hansmann, B. J. Whelan, B. Kaminsky, B. Riedel, B. Ruzybayev, C. Arguelles, C. Bohm, C. De Clercq, C. Finley, C. Ha, C. Haack, Ch. Weaver, C. H. Wiebusch, C. Kopper, C. P\\'erez de los Heros, C. Pfendner, C. Rott, C. Spiering, C. Walck, C. Wendt, C. Wichary, D. Altmann, D. Berley, D. Bindig, D. Bose, D. Chirkin, D. F. Cowen, D. Gier, D. G\\'ora, D. Grant, D. Hebecker, D. Heereman, D. Hellwig, D. J. Boersma, D. J. Koskinen, D. L. Xu, D. Pieloth, D. R. Nygren, D. R. Williams, D. Ryckbosch, D. Seckel, D. Soldin, D. Tosi, D. Z. Besson, E. A. Strahler, E. Beiser, E. Bernardini, E. Blaufuss, E. Cheung, E. Jacobi, E. Middell, E. Middlemas, E. Pinat, E. Resconi, E. Unger, F. Bos, F. Halzen, F. Huang, F. McNally, F. Scheriau, G. Binder, G. C. Hill, G. de Wasseige, G. Golup, G. Kohnen, G. Kroll, G. Maggi, G. Merino, G. M. Spiczak, G. S. Japaridze, G. Te\\v{s}i\\'c, G. T. Przybylski, G. W. Sullivan, G. Yodh, H. Dembinski, H.-G. Sander, H. Kolanoski, H. Niederhausen, H. Pandya, H.-P. Bretz, H. S. Matis, H. Taavola, H. Wissing, IceCube Collaboration: M. G. Aartsen, I. Taboada, J. A. Aguilar, J. Adams, J. A. Pepper, J. Auffenberg, J. Becker Tjus, J. Blumenthal, J. Braun, J. Casey, J. C. Davis, J. C. D\\'iaz-V\\'elez, J. C. Groh, J. Daughhetee, J. Feintzeig, J. Felde, J. Gallagher, J. G. Gonzalez, J. Hignight, J. J. Beatty, J. Kemp, J. Kiryluk, J. Kl\\\"as, J. Kunnen, J. Leuner, J. L. Kelley, J. L. Lanfranchi, J. L\\\"unemann, J. Madsen, J. Miller, J. P. A. M. de Andr\\'e, J. P. Dumm, J. Posselt, J. P\\\"utz, J. P. Yanez, J. Sandroos, J. Vandenbroucke, J. van Santen, J. Veenkamp, K. Abraham, K. B. M. Mahn, K. Clark, K. D. de Vries, K. D. Hoffman, K. Filimonov, K. Ghorbani, K. Hanson, K.-H. Becker, K. Helbing, K. Holzapfe, K. Hoshina, K. Hultqvist, K. Jero, K. Krings, K. Mase, K. Meagher, K. Rawlins, K. Schatto, K. Wiebe, K. Woschnagg, L. Brayeur, L. Classen, L. Gerhardt, L. Gladstone, L. K\\\"opke, L. Mohrmann, L. Paul, L. R\\\"adel, L. 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Nowicki, S. Coenders, S. De Ridder, S. Euler, S. Fahey, S. Flis, S. Hickford, S. In, S. Kopper, S. Miarecki, S. M. Saba, S. Richter, S. R. Klein, S. Robertson, S. Sarkar, S. Schoenen, S. Sch\\\"oneberg, S. Seunarine, S. Ter-Antonyan, S. Tilav, S. Vallecorsa, S. Vanheule, S. W. Barwick, S. Westerhoff, S. Yoshida, T. Anderson, T. C. Arlen, T. DeYoung, T. Ehrhardt, T. Fischer-Wasels, T. Fuchs, T. Gl\\\"usenkamp, T. Karg, T. K. Gaisser, T. Kuwabara, T. Menne, T. Meures, T. Montaruli, T. Palczewski, T. Ruhe, T. R. Wood, T. Schmidt, T. Stanev, T. Stezelberger, U. Naumann, V. Baum, W. Huelsnitz, W. Rhode, X. Bai, X. W. Xu, Y. Xu","submitted_at":"2015-05-27T10:34:40Z","abstract_excerpt":"The Milky Way is expected to be embedded in a halo of dark matter particles, with the highest density in the central region, and decreasing density with the halo-centric radius. 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