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Activity report from CAF group. Marcello , Davide , Pigi , Camilo , Salvatore, Orso , David, Silvia, Georgi , Anna, Haiyun. CAF strategy. What kind of data do we have ? Minimum Bias (low P T muon mostly from secondary vertex) Beam Halo (horizontal muon tracks) Cosmic - PowerPoint PPT Presentation
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Activity report from CAF group
Marcello, Davide, Pigi, Camilo, Salvatore, Orso, David, Silvia, Georgi, Anna, Haiyun
CAF strategy• What kind of data do we have ?– Minimum Bias (low PT muon mostly from secondary vertex)
– Beam Halo (horizontal muon tracks)– Cosmic
• What we can study with those events ?– Noise and occupancy– Endcap efficiency
• EVENT SELECTION• STUDIES
What we are doing now ?
• Beam Halo selection– Trigger based (Salvatore) ready– CSC segment based (Haiyun) almost ready
• Minimum Bias selection– RPC rechits + tracker tracks (Orso)
• Detector Studies– RecHits distributions with MB and Cosmic (Orso)– CSC/RPC correlation (Camillo, Haiyun, Georgi)– Efficiency with beam halo events (Camillo)
• Trigger Studies: CSC versus RPC (Maciek)
• Noise (Silvia, David and shifter)
• BX distribution (Anna and Pigi)
Beam Splashes
"noisy strip" state:strip occupancy 3.5 times greater than average occupancy (from roll occupancy histogram)"noisy chamber”: average multiplicity > 6
Noise History from DQM(David Lomidze)
Historical DQM is on the way
CSC – RPC correlations(Camillo & Pigi)
BX distribution - splashes
Roll: RE+2_R3_CH02_CRoll: RE+2_R3_CH20_BRoll: RE+2_R3_CH20_CRoll: RE+2_R3_CH03_CRoll: RE+2_R3_CH21_CRoll: RE+2_R2_CH22_CRoll: RE+2_R2_CH29_BRoll: RE+2_R2_CH29_CRoll: RE+3_R2_CH20_ARoll: RE+3_R2_CH15_BRoll: RE+3_R2_CH16_BRoll: RE+3_R3_CH06_BRoll: RE+3_R3_CH06_CRoll: RE+3_R3_CH36_BRoll: RE+3_R3_CH36_C
Bunch crossing studiesfrom DQM(Anna C. & Pigi)
Minimum Bias muon
Minimum Bias muon