ITEDA   22747
INSTITUTO DE TECNOLOGIA EN DETECCION Y ASTROPARTICULAS
Unidad Ejecutora - UE
congresos y reuniones científicas
Título:
AMIGA Status Report
Autor/es:
N. ACCIALINI, A. ALMELA, D. ALONSO, F. BARABÁS, P. BUCHHOLZ, U. FRÖHLICH, Y. KOLOTAEV, M. NIECHCIOL, M. PONTZ,; A. CANCIO, R. CARUSO, F. CONTRERAS, G. DE INNOCENTI, G. DE LA VEGA, L. DEL PERAL, A. ETCHEGOYEN, P. FITZELEW, A. FUSTER,; F. GALLO, R. GAMARRA, B. GARCÍA, M. GÓMEZ BERISSO, N. GONZÁLEZ, D. GORBEÑA, M. R. HAMPEL, M. JOSEBACHUILI, A. KAKAZU,; J. KLEINFELLER, A. KRIEGER, A. LUCERO, A. MANCILLA, J. MAYA, P. MAZUR, D. MELO, M. PLATINO, E. PONSONE,; D. RAVIGNANI, C. REYES, D. RIPETOUR CHAIMAN, M. RISSE, M. D. RODRÍGUEZ-FRÍAS, G. ROS, F. SÁNCHEZ, A. SEDOSKI CROCE, M. SETTIMO,; I. SIDELNIK, F. SUAREZ, A. TAPIA CASANOVA, R. TCACIUC, M. TIGGES, C. VARELA, M. VIDELA, O. WAINBERG, B. WUNDHEILER, D. YELOS
Reunión:
Encuentro; Pierre Auger Internal GAP Note Nº 2011-120; 2011
Resumen:
AMIGA will allow the lowering of the Auger energy threshold of the surface detector down 1017 eV (433 and 750 m detector spacing arrays, see Figure 1.1) with muon data covering at least the 3 – 20 EeV range with the currently approved 750 m array. The coincident measurement of events with hybrid-fluorescence detectors (FD), surface detectors (SD), and muon detector (MD) techniques will position the Auger data as ultimate from 1017 eV onwards.