Fixed, com2019, Sat Apr 6 08:18:55 2019, mugast, RUN, Software, CD2, Online Scalers run 256 @8h00 am 06/04 for reference 
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Fixed, com2019, Sat Apr 6 10:57:35 2019, Nicolas, OFFLINE, Software, CD2, time of flight v.s. energy in MUGAST (run 256, all stat)
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Fixed, com2019, Sat Apr 6 11:40:08 2019, mugast, OFFLINE, Software, CD2, AGATA spectrum in coincidence with MUGAST VAMOS run 256
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Fixed, com2019, Sun Apr 7 14:24:18 2019, Valerian, OFFLINE, Software, CD2, Ex and E gamma with all statistic (run 256+257)
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Fixed, com2019, Tue Apr 9 10:44:40 2019, Valerian, MUST2, Software, CD2, CsI Calib files from the commissioning for proton
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| CsI calibration obtained from the proton data of the commissioning of mugast. |
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Fixed, e744s, Tue Apr 9 18:08:22 2019, Marlène and François, DAQ, Software, , new inputs in the ADC Mugast
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new inputs in the ADC mugast
T_Mugast_HF = input N°2
E_AGATA = agata 42 = input N°3
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Pinned, e744s, Wed Apr 10 11:57:37 2019, A. Lemasson, OFFLINE, Software, , VAMOS Conversion HowTo
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[B]HOW TO convert a run in VAMOS[/B]
[LIST]
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Pinned, e786s, Wed Apr 10 13:30:48 2019, Valerian, Adrien and Antoine (edit by Louis), OFFLINE, Software, N/A, How to perform analysis for e786s
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[U][B]
Here is the updated procedure to convert a run, with VAMOS data and add those data to the Kinematic plot.
[/B][/U]
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Fixed, e744s, Thu Apr 11 11:36:09 2019, Valerian, OFFLINE, Software, CH2, Comparison between the two e744
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| Current calibration is off, a shift of -1.5MeV was done to reproduce the previous data. |
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Fixed, e744s, Thu Apr 11 13:43:26 2019, Valerian, OFFLINE, Software, CH2, Target position for 14N runs
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Fixed, e744s, Thu Apr 11 16:07:59 2019, Valerian and Louis, OFFLINE, Software, CH2, HF resolution
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| Using the value of the HF=83,4ns. We can obtain the calibrated plot of T_CATS2_HF which is joined and gives us roughly a 2-3 ns resolution for the HF |
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Fixed, e744s, Thu Apr 11 18:20:27 2019, Valerian and Diego, OFFLINE, Software, CH2, Timing issue between vamos and mugast
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A cut is seen on the TAC between MUGAST and the focal plane multiwire of VAMOS when one select XF or DC0_Y>-1500
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Fixed, e744s, Fri Apr 12 10:12:45 2019, Valerian, OFFLINE, Software, CH2, Comparison between HF and CATS for ELab ThetaLab
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| Using the HF show noises that is not seen with CATS on the ToF spectra |
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Fixed, e744s, Fri Apr 12 14:13:11 2019, Giuseppe D'Agata, OTHER, Software, N/A, Converted runs
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Runs additionally converted up to now:
70
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Fixed, e744s, Fri Apr 12 19:44:09 2019, diego, VAMOS, Software, , SetAlias script for VAMOS identification
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Fixed, e744s, Fri Apr 12 22:44:43 2019, Valerian and Diego, OFFLINE, Software, CH2, 13N measured in Vamos do correspond to protons events in MUST2
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| Doing a cut on M vs M/Q corresponding to 13N one can see that most of the events do correspond to protons events in MUST2!!! |
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Fixed, e744s, Sat Apr 13 00:27:08 2019, iulian nicolas Nikola Mariluz, RUN, Software, CH2, Screenshots run119 v1 21x
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Fixed, e744s, Sat Apr 13 22:45:27 2019, Beyhan, Sylvain, Jaromir, AGATA, Software, N/A, Agata yellow phase 1 minute
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Agata yellow 1 minute
All the trigers emitted by (every) single crystal were refused by ACQ for 1 minute.
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Fixed, e744s, Sat Apr 13 23:19:57 2019, Valerian, Freddy, Iulian and Fairouz, OFFLINE, Software, CH2, Very preliminary results for two protons
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| Join are very preliminary spectra for the two protons events gated on 13N in VAMOS with a multiplicity 1 event in MUST2. This condition adds a lot of noise. |
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Fixed, e744s, Sun Apr 14 12:11:52 2019, Valerian and Iulian, OFFLINE, Software, CH2, VERY VERY preliminary results Gamma-p
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Around 8-10 events are found in the good energy vs Brho region and Si_T vs Si_E region for the gamma emission.
Joined are :
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