Publications [#304607] of Kate Scholberg

Papers Published
  1. Ambrosio, M; Antolini, R; Aramo, C; Auriemma, G; Baldini, A; Barbarino, GC; Barish, BC; Battistoni, G; Bellotti, R; Bemporad, C; Bernardini, P; Bilokon, H; Bisi, V; Bloise, C; Bower, C; Bussino, S; Cafagna, F; Calicchio, M; Campana, D; Carboni, M; Castellano, M; Cecchini, S; Cei, F; Chiarella, V; Choudhary, BC; Coutu, S; De Benedictis, L; De Cataldo, G; Dekhissi, H; De Marzo, C; De Mitri, I; Derkaoui, J; De Vincenzi, M; Di Credico, A; Erriquez, O; Favuzzi, C; Forti, C; Fusco, P; Giacomelli, G; Giannini, G; Giglietto, N; Giorgini, M; Grassi, M; Gray, L; Grillo, A; Guarino, F; Guarnaccia, P; Gustavino, C; Habig, A; Hanson, K; Heinz, R; Huang, Y; Iarocci, E; Katsavounidis, E; Kearns, E; Kim, H; Kyriazopoulou, S; Lamanna, E; Lane, C; Levin, DS; Lipari, P; Longley, NP; Longo, MJ; Maaroufi, F; Mancarella, G; Mandrioli, G; Manzoor, S; Neri, AM; Marini, A; Martello, D; Marzari-Chiesa, A; Mazziotta, MN; Mazzotta, C; Michael, DG; Mikheyev, S; Miller, L; Monacelli, P; Montaruli, T; Monteno, M; Mufson, S; Musser, J; Nicoló, D; Orth, C; Osteria, G; Ouchrif, M; Palamara, O; Patera, V; Patrizii, L; Pazzi, R; Peck, CW; Petrera, S; Pistilli, P; Popa, V; Pugliese, V; Rainò, A; Reynoldson, J; Ronga, F; Rubizzo, U; Satriano, C; Satta, L; Scapparone, E; Scholberg, K; Sciubba, A; Serra-Lugaresi, P; Severi, M; Sioli, M; Sitta, M; Spinelli, P; Spinetti, M; Spurio, M; Steinberg, R; Stone, JL; Sulak, LR; Surdo, A; Tarlè, G; Togo, V; Ugolotti, D; Vakili, M; Walter, CW; Webb, R, Observation of the shadowing of cosmic rays by the Moon using a deep underground detector, Physical Review D, vol. 59 no. 1 (November, 1998), pp. 1-7 [doi] .

    Abstract:
    Using data collected by the MACRO experiment during the years 1989-1996, we show evidence for the shadow of the Moon in the underground cosmic ray flux with a significance of 3.6σ. This detection of the shadowing effect is the first by an underground detector. A maximum-likelihood analysis is used to determine that the angular resolution of the apparatus is 0.9°±0.3°. These results demonstrate MACRO'S capabilities as a muon telescope by confirming its absolute pointing ability and quantifying its angular resolution. ©1998 The American Physical Society.