AIDA
GELINA
BRIKEN
nToF
CRIB
ISOLDE
CIRCE
nTOFCapture
DESPEC
DTAS
EDI_PSA
179Ta
CARME
StellarModelling
DCF
K40
AIDA
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Offline analysis of R25_11 to _13 see http://ribf-exp.riken.jp/elog/RIBF123/141 "F5 C target F7 no F11 C 6mm Date 2016/11/10 Start time: 08:20 DLT File: 161110_0820_767778Ni_035.dlt RUN: 035 Aida RUN: R25_11 Comment: F11 Degraders taken out after few minutes Degrader: no Rates: F11R: 450 Hz BRIKEN: 200 Hz Stop time: 09:18 AIDA run: R25_23 ROOT file: 161110_0918_767778Ni_035.root" Attachments 1-3 show spectra s2130-s2135 over different ranges s2130 DSSSD #1 time between successive HEC events (2.56us/channel) : : s2135 DSSSD #6 time between successive HEC events (2.56us/channel) Attachment 4 s2000-s2005 DSSSD #1-6 LEC m_p versus m_n Attachment 5 s2100-s2105 DSSSD #1-6 HEC m_p versus m_n HEC events for each DSSSD are defined as m_p_hec > 0 and m_n_hec > 0 Minimum time between HEC events = 16 channels = 40.96us Centroid channels 0-65525 of spectrum s2130 = ch 2566.44 => 0.00657s -> 152Hz which agrees well with the typical DSSSD #1 rate for these data files Is there structure at channel 30 => 76.8us ? More likely it shows variations in readout time from HEC event to HEC event.
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