Mathematical Institute

Observation of the cosmic-ray shadow of the Moon with IceCube

Collaboration, I Aartsen, M Abbasi, R Abdou, Y Ackermann, M Adams, J Aguilar, J Ahlers, M Altmann, D Auffenberg, J Bai, X Baker, M Barwick, S Baum, V Bay, R Beatty, J Bechet, S Tjus, J Becker, K Bell, M Benabderrahmane, M BenZvi, S Berdermann, J Berghaus, P Berley, D Bernardini, E Bernhard, A Bertrand, D Besson, D Binder, G Bindig, D Bissok, M Blaufuss, E Blumenthal, J Boersma, D Bohaichuk, S Bohm, C Bose, D Böser, S Botner, O Brayeur, L Bretz, H Brown, A Bruijn, R Brunner, J Carson, M Casey, J Casier, M Chirkin, D Christov, A Christy, B Clark, K Clevermann, F Coenders, S Cohen, S Cowen, D Silva, A Danninger, M Daughhetee, J Davis, J Clercq, C Ridder, S Desiati, P With, M DeYoung, T Díaz-Vélez, J Dunkman, M Eagan, R Eberhardt, B Eisch, J Ellsworth, R Euler, S Evenson, P Fadiran, O Fazely, A Fedynitch, A Feintzeig, J Feusels, T Filimonov, K Finley, C Fischer-Wasels, T Flis, S Franckowiak, A Franke, R Frantzen, K Fuchs, T Gaisser, T Gallagher, J Gerhardt, L Gladstone, L Glüsenkamp, T Goldschmidt, A Golup, G Gonzalez, J Goodman, J Góra, D Grandmont, D Grant, D Groß, A Ha, C Ismail, A Hallen, P Hallgren, A Halzen, F Hanson, K Heereman, D Heinen, D Helbing, K Hellauer, R Hickford, S Hill, G Hoffman, K Hoffmann, R Homeier, A Hoshina, K Huelsnitz, W Hulth, P Hultqvist, K Hussain, S Ishihara, A Jacobi, E Jacobsen, J Jagielski, K Japaridze, G Jero, K Jlelati, O Kaminsky, B Kappes, A Karg, T Karle, A Kelley, J Kiryluk, J Kislat, F Kläs, J Klein, S Köhne, J Kohnen, G Kolanoski, H Köpke, L Kopper, C Kopper, S Koskinen, D Kowalski, M Krasberg, M Krings, K Kroll, G Kunnen, J Kurahashi, N Kuwabara, T Labare, M Landsman, H Larson, M Lesiak-Bzdak, M Leuermann, M Leute, J Lünemann, J Madsen, J Maruyama, R Mase, K Matis, H McNally, F Meagher, K Merck, M Mészáros, P Meures, T Miarecki, S Middell, E Milke, N Miller, J Mohrmann, L Montaruli, T Morse, R Nahnhauer, R Naumann, U Niederhausen, H Nowicki, S Nygren, D Obertacke, A Odrowski, S Olivas, A Olivo, M O'Murchadha, A Paul, L Pepper, J Heros, C Pfendner, C Pieloth, D Pinat, E Pirk, N Posselt, J Price, P Przybylski, G Rädel, L Rameez, M Rawlins, K Redl, P Reimann, R Resconi, E Rhode, W Ribordy, M Richman, M Riedel, B Rodrigues, J Rott, C Ruhe, T Ruzybayev, B Ryckbosch, D Saba, S Salameh, T Sander, H Santander, M Sarkar, S Schatto, K Scheel, M Scheriau, F Schmidt, T Schmitz, M Schoenen, S Schöneberg, S Schönwald, A Schukraft, A Schulte, L Schulz, O Seckel, D Sestayo, Y Seunarine, S Sheremata, C Smith, M Soldin, D Spiczak, G Spiering, C Stamatikos, M Stanev, T Stasik, A Stezelberger, T Stokstad, R Stößl, A Strahler, E Ström, R Sullivan, G Taavola, H Taboada, I Tamburro, A Tepe, A Ter-Antonyan, S Tešić, G Tilav, S Toale, P Toscano, S Usner, M Drift, D Eijndhoven, N Overloop, A Santen, J Vehring, M Voge, M Vraeghe, M Walck, C Waldenmaier, T Wallraff, M Wasserman, R Weaver, C Wellons, M Wendt, C Westerhoff, S Whitehorn, N Wiebe, K Wiebusch, C Williams, D Wissing, H Wolf, M Wood, T Woschnagg, K Xu, C Xu, D Xu, X Yanez, J Yodh, G Yoshida, S Zarzhitsky, P Ziemann, J Zierke, S Zoll, M Phys. Rev. D volume 89 102004 (29 May 2013) https://arxiv.org/abs/1305.6811v1