LHCf is a collider experiment dedicated to obtaining information relevant to ultra-high-energy cosmic-ray physics. One of the two LHCf detectors has position-sensitive silicon microstrip layers that are read out with front end electronics. These electronics saturate for high energy photon showers because of the limited dynamic range of the preamplifier. Consequently we are planning an upgrade of the processing circuits in anticipation of LHC operation at increased collision energy, and we are developing an analysis method to correct for the saturation effect. An overview of these data analysis methods will be given in this paper.

Data analysis of the LHCf Si microstrip sensors / Noda, K.; Adriani, O.; Bonechi, L.; Bongi, M.; Castellini, G.; D'Alessandro, R.; Fukatsu, K.; Haguenauer, M.; Itow, Y.; Kasahara, K.; Kawade, K.; Macina, D.; Mase, T.; Masuda, K.; Menjo, H.; Mitsuka, G.; Muraki, Y.; Nakai, M.; Papini, P.; Perrot, A.-L.; Ricciarini, S.; Sako, T.; Shimizu, Y.; Suzuki, K.; Suzuki, T.; Taki, K.; Tamura, T.; Torii, S.; Tricomi, A.; Turner, W.C.. - ELETTRONICO. - 5:(2011), pp. 35-38. (Intervento presentato al convegno 32nd International Cosmic Ray Conference, ICRC 2011 tenutosi a Beijing, chn nel 2011) [10.7529/ICRC2011/V05/0421].

Data analysis of the LHCf Si microstrip sensors

Noda, K.;ADRIANI, OSCAR;BONGI, MASSIMO;D'ALESSANDRO, RAFFAELLO;
2011

Abstract

LHCf is a collider experiment dedicated to obtaining information relevant to ultra-high-energy cosmic-ray physics. One of the two LHCf detectors has position-sensitive silicon microstrip layers that are read out with front end electronics. These electronics saturate for high energy photon showers because of the limited dynamic range of the preamplifier. Consequently we are planning an upgrade of the processing circuits in anticipation of LHC operation at increased collision energy, and we are developing an analysis method to correct for the saturation effect. An overview of these data analysis methods will be given in this paper.
2011
Proceedings of the 32nd International Cosmic Ray Conference, ICRC 2011
32nd International Cosmic Ray Conference, ICRC 2011
Beijing, chn
2011
Noda, K.; Adriani, O.; Bonechi, L.; Bongi, M.; Castellini, G.; D'Alessandro, R.; Fukatsu, K.; Haguenauer, M.; Itow, Y.; Kasahara, K.; Kawade, K.; Macina, D.; Mase, T.; Masuda, K.; Menjo, H.; Mitsuka, G.; Muraki, Y.; Nakai, M.; Papini, P.; Perrot, A.-L.; Ricciarini, S.; Sako, T.; Shimizu, Y.; Suzuki, K.; Suzuki, T.; Taki, K.; Tamura, T.; Torii, S.; Tricomi, A.; Turner, W.C.
File in questo prodotto:
Non ci sono file associati a questo prodotto.

I documenti in FLORE sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.

Utilizza questo identificatore per citare o creare un link a questa risorsa: https://hdl.handle.net/2158/1088315
Citazioni
  • ???jsp.display-item.citation.pmc??? ND
  • Scopus 2
  • ???jsp.display-item.citation.isi??? ND
social impact