The analog signal processor of the Auger fluorescence detector prototype
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Lodovico Ratti | V. Speziali | D. V. Camin | P. P. Trapani | E. Menichetti | P. Privitera | R. Gariboldi | V. Grassi | Valerio Re | R. Fonte | M. Lapolla | L. Ratti | V. Re | V. Speziali | V. Grassi | P. Privitera | E. Menichetti | P. Manfredi | P. Trapani | D. Camin | P. Cattaneo | R. Fonte | M. Destro | S Argirò | Pw Cattaneo | M Destro | Pf Manfredi | M Nicotra | M. Lapolla | R. Gariboldi | S. Argirò | M. Nicotra
[1] D. V. Camin,et al. Monitoring DC anode current of a grounded-cathode photomultiplier tube , 1999 .
[2] Robert O. Reid,et al. The cosmic ray energy spectrum above 4*1017 eV as measured by the Haverah Park array , 1991 .
[3] L. Ratti,et al. A bilinear analog compressor to adapt the signal dynamic range in the AUGER fluorescence detector , 2001 .
[4] J. W. Elbert,et al. The Cosmic ray energy spectrum observed by the Fly's Eye , 1994 .
[5] M. Teshima,et al. The cosmic ray energy spectrum above 3 × 1018 eV measured by the Akeno Giant Air Shower Array , 1995 .
[6] John Linsley,et al. Evidence for a primary cosmic-ray particle with energy 10**20-eV , 1963 .