Fixed, e768s, Tue Jul 16 21:30:19 2019, Chloe Fougeres, OTHER, General, LiF, PACE4 fusion-evaporation 
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| Simulated yields with beams 15N and 15O (4.7 MeV/u) on target LiF. |
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Fixed, e744s, Mon Apr 8 14:41:07 2019, Daniele M, OTHER, General, N/A, PACE4 cross check ------ E744s to-do list , proposal and other relevant documents
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Fusion-evaporation calculation cross-check:
angular range [10-40]deg
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Fixed, com2019, Fri Apr 5 19:42:28 2019, Jenn Sanchez & Ana Montaner-Pizá, OTHER, General, CD2, PACE4 calculations
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Attached you can find the PACE4 calculations for the reactions 16O + 12C and 16O + d at 6 MeV/u beam.
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Fixed, e768s, Tue Jul 16 22:25:51 2019, mugast, OTHER, General, , Oxygen 15 decay scheme
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beta+ decay to the ground state of 15N
gammas @ 511 keV |
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Pending, TEST, Tue Jan 21 17:55:12 2020, Marlène, MUST2, Hardware, , Ovv error on the -5V of CAEN boards
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The Ovv error shows on the -5V (first one) of the 3 board (5,3.3,10V for MUST2§squares)
It means that the voltage is over the asked value.
If we ask 5V, we get 5.5V in reality
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Fixed, e768s, Fri Jul 19 08:09:21 2019, Jenn, Kseniia, OTHER, General, , Overview nightshift run 112
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Smooth night, everything was working properly.
Checked agata rootfile to see preliminary gammas.
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Fixed, com2019, Sun Apr 7 21:35:51 2019, Valerian, Freddy and Antoine, RUN, General, N/A, Overnight run259 crashed during the night
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Run 259 which was an overnight run crashed (During the night between the 6 and the 7th of April).
The result of this crash was that the the acquisition started writing a 4gb file each seconds for 80 seconds. We then had to remove the run (~300gb) as |
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Fixed, e744s, Mon Apr 15 15:18:55 2019, A. Lemasson, VAMOS, Hardware, , Optimization of IC Shaping
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During Run 129,
1) investigation of the trapezoidal filter of IC
2) The Conclusion is that if we reduce the shaping to 2.5 us we reduce the random line in IC vs IC (At 1e5 in VAMOS : Random Line / Peak is 18.5 % compared |
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Fixed, e744s, Tue Apr 16 00:01:43 2019, louis, Guiseppe, ONLINE, General, CH2, Online snapshot from run 132 20x
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| Online snapshot from run 132 |
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Fixed, com2019, Sat Apr 6 02:48:39 2019, Iulian Ruxandra, RUN, Software, , Online Spectra run 256 @2h30 am 06/04 (for reference) 11x
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The online spectra (for reference)
No timing on Mg3 & Mg4 side X. Those correspond with the masked channels on the Muvi1 |
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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 02:52:51 2019, Iulian Ruxandra, RUN, Software, , Online Scalers run 256 @2h30 am 06/04 for reference
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Fixed, e786s, Wed Jun 12 17:59:01 2019, mugast, OTHER, Software, , Online Energy Calibration
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| Updated Online Energy calibration for MUGAST, based on run_0231 data |
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Fixed, e786s, Wed Jun 12 18:11:04 2019, mugast, OTHER, Software, , Online Energy Calibration
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Fixed, e793s, Fri Mar 12 09:52:01 2021, mugast (Sarah, Louis), OFFLINE, General, CD2, Offline analysis run up to 56 8am
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1) A high energy gamma has been identified at 3505 keV by gating on 3-5 MeV range in excitation energy. This transition is unknown so far
2) preliminary angular distribution has been extracted for the p states(<1MeV) and the f states (3-5MeV) corrected from geometrical efficiency. Angular |
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Fixed, e786s, Wed Jun 26 05:58:23 2019, Freddy, OFFLINE, General, N/A, Offline analysis run 56 and 58
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Fixed, e786s, Tue Jun 25 02:46:32 2019, Sylvain, Louis, OFFLINE, General, Cryo-3He, Offline analysis run 56
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Offline analysis of run 56 has been perfomed. On plots, kinematics lines and excitation energy are shown using gate on 47K in vamos. Then agata spectra
is shown using gate on 47K in VAMOS un valid event in MUGAST. One can (may be) distinguish a peak at 368keV... |
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Fixed, e793s, Sat Mar 13 10:11:44 2021, Adrien, OFFLINE, General, CD2, Offline analysis of run 51-61
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Run 51 to 61 are converted and analysed.
I fixed the gamma/no gamma normalisation after binning change.
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Fixed, e793s, Wed Mar 10 22:19:22 2021, Adrien, Freddy, Wilton and Nigel, OFFLINE, General, CD2, Offline analysis of run 51 and 52 using ganil files
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We noted that the gamma ray efficiency calculated from file converted from AGATA was close 100%. We concluded that the conversion program was reauiring
a gamma ray to be present.
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Fixed, e786s, Mon Jun 24 06:14:02 2019, Louis, OFFLINE, General, Cryo-3He, Offline analysis 46Ar(3He,d)47K for run 49
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Energy loss vs. Time of Flight identification has been performed in mugast. On can notice some calibration trouble in energy and time. Big shift of the
deToF bananas are seen from one telescope to an other. Furthermore, one can distinguish proton and deuteron in MG1, 3 and 4 but it's it's very difficult
to conclude for 5,7 and 11.
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