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AIDA
GELINA
BRIKEN
nToF
CRIB
ISOLDE
CIRCE
nTOFCapture
DESPEC
DTAS
EDI_PSA
179Ta
CARME
StellarModelling
DCF
K40
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AIDA |
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Message ID: 457
Entry time: Wed Nov 16 06:47:02 2016
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Author: |
TD |
Subject: |
Analysis of data files R25_11 to _13 |
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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)
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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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