MUST2
SAMURAI_2018
S3-LEB-LPC
SUPERNEMO
MUGAST
EXPAND
SCALP
GALATRON
HiCARI
VELO
|
MUGAST, Page 11 of 132 |
Not logged in |
|
|
Status |
ExpNbr |
Date |
Author |
Type |
Category |
Target-Source |
Subject |
Fixed | e768s |
Wed Jul 24 14:41:09 2019 |
mugast | RUN | General | N/A | VAMOS divison 30 | VAMOs division is set to 30 |
Fixed | e768s |
Tue Jul 23 16:19:14 2019 |
Marlène | OTHER | Hardware | | VAMOS division | VAMOS division was set 10 instead of 100.
CATS 1 & CATS2 scalers are sent to the two last channels of the scaler |
Fixed | e768s |
Fri Jul 26 15:47:17 2019 |
mugast | VAMOS | Hardware | LiF | VAMOS division | New VAMOS division : 10. |
Fixed | e744s |
Thu Apr 11 02:36:15 2019 |
Daniele, Andrea | VAMOS | General | N/A | VAMOS cfg |
VAMOS BRO= 0.64050 Phi= 45 Dtrans= 0.66m T-xFoc=7.995m
| Objects | Name | Settings | Actual
| VAMOS_FAIS_IN | VAMOS_BRO_IN | 0.640500 | 0.0
| | VAMOS_W_IN | 4.934969 | 3.258E+36
| | VAMOS_ION_A | 14.000 | 3.336E+36
| | VAMOS_ION_AM_IN | 14.003074 | 0.0
| | VAMOS_ION_Q | 7.00 | 0.0
| | VAMOS_ION_Z | 7.00 | 0.0
| G1_Q41 | G1.G.Q41 | 170.713 | 170.776
| | G1_Q41_G | -1.643 | -1.643
| G1_Q42 | G1.G.Q42 | 251.022 | 251.112
| | G1_Q42_G | 0.732 | 0.732
| G1_DVFW | G1.G.DVFW | 0.0 | 0.0
| G1_FW_HTP | G1.G.FW.HTP | 0.0 | 0.002
| G1_FW_HTN | G1.G.FW.HTN | 0.0 | 0.002
| G1_DVFW_HALL | G1.G.DVFW.HALL | 0.0 | 0.0
| G1_D41 | G1.G.D4.P | 215.598 | 216.160
| | G1.G.D41.RMN | 3249.630 | 3249.630
|
|
Fixed | e793s |
Wed Mar 17 07:18:39 2021 |
Laetitia, Charlie | ONLINE | General | CD2 | VAMOS acquisition stopped | The acquisition on Vamos get stucked at 6h49. At 07:18, we stopped and started a new run (run 64) |
Fixed | e793s |
Wed Mar 17 07:25:24 2021 |
Laetitia, Charlie | ONLINE | General | CD2 | VAMOS acquisition stopped | Vamos acquisition get stucked at 6h49 (with 2 Gbit). We stopped and started a new run at 07h18 (Run #64) |
Fixed | e768s |
Sat Jul 20 23:57:34 2019 |
Diego | OFFLINE | General | | VAMOS acceptance, comparison between 9+ and 10+ states | Figures above, simulation of VAMOS acceptance for 10+ and 9+ 19Ne charge states. Ratio between them quite big (0.58)
Figures below, comparison of the states with offline data. Ratio much smaller.
It seems like acceptance doesn't cut the 10+ charge state too much, but 10+ is less produced than 9+. |
Fixed | e786s |
Sun Jun 23 09:06:29 2019 |
Daniele M | VAMOS | General | N/A | VAMOS SETTINGS | attached the energy measured in CIME and the calculated VAMOS settings |
Pinned | e744s |
Wed Apr 10 11:57:37 2019 |
A. Lemasson | OFFLINE | Software | | VAMOS Conversion HowTo |
HOW TO convert a run in VAMOS
- Do : source $HOME/GoToVamosAna
- To Convert a Run : MyVAna -d2Ar <RunNr>
- Otherwise, If you want to convert a single file : MyVAna -d2Ar -f <Infile> <OutFile>
- Output Root rile is written to : ./RootA/
If you encounter the error on Brho "Could not find the BrhoRef for the run <RunNr> ", Update the ./Calibs/ListBrho.dat file with relevant Brho for RunNr |
Fixed | e786s |
Tue Jun 25 15:33:40 2019 |
A Lemasson | VAMOS | General | | VAMOS Analysis - Brho | VAMOS Analysis :
VAMOS PID with attached SetAlias.C
Suggestion to change Brho from 1.05 to 0.95 based on the distribution of K ions to optimize acceptance on the K
ions |
Fixed | e768s |
Wed Jul 24 17:21:27 2019 |
Diego | OTHER | General | | VAMOS Acceptance with different positions of the beam in the target | |
Fixed | e793s |
Sun Mar 14 15:20:47 2021 |
Adrien | OFFLINE | General | CD2 | Updated Angular distribution macro | The angular distribution macro has been updated and now produce TWOFNR calculation on the fly.
Feel free to add new plots and play around with the parameter.
MakePlot will produce the distribution using Ex and sigmaEx of the state and Eg and sigmaG of the gamma. Efficiency is automatically taken into account using the efficiency provided by manu.
FIT will perform the TWOFNR calculation using The energy of the state, l and j of the transferred nucleon and J of the formed states. Once the calculation done, it does the fit to the data and extract the C2S.
I found the number strangely small so I suspect we do something wrong.
To run it:
Open a terminal
$> lpcgrit
$> npp MUGAST
$> cd e793s
$> root AngDist.C |
Fixed | e768s |
Sun Jul 28 08:20:38 2019 |
Sylvain & Franco | RUN | General | | Update on possible restart | The problem that caused the interruption was due to a failure in the cooling system.
The last update we've had is that we might have the beam back not before late afternoon.
We will keep you updated. |
Fixed | e768s |
Sun Jul 28 16:23:48 2019 |
Nicolas | RUN | General | | Update on possible restart | Same situation as before lunch, the beam is still in C0 and not yet in CSS1. We may have beam in late evening.... |
Ongoing | e768s |
Sun Jul 28 19:58:57 2019 |
Nicolas | RUN | General | | Update on possible restart | Beam is now at the exit of CSS2 though We may have beam around midnight.... |
|
Fixed | e768s |
Sun Jul 28 21:59:43 2019 |
Nicolas | RUN | General | | Update on possible restart |
Beam is in G1 with 3e6 pps. PCP will optimize for about 1-1,5h before we take the beam. |
Fixed | TEST |
Wed Mar 11 18:12:40 2020 |
Marlène & Franco | GRIT | Hardware | N/A | Update on Mugast |
(Probably) final update of the status of the detector before the experiment:
- MG5 does not trigger on Y (no pulser, no alpha source). This can explain why in the last experiment we could not run the time calibration of its Y.
- We changed kapton on MG7 but we still miss the same part of the detector. This points to a problem of the board...
- There is nothing we can do for the moment for MG11, the re-bounding would take too long. We will keep it like this.
- MUST2 detectors have higher current than usual but the signals from alpha source are fine.
- MM1 was changed but still shows the problem of the fluctuation of current. We also tried to change the HV supply (now it's on MG6) but nothing changes. This also seems to point to a problem of the board...
- We noted that, with circulation of alcool-water liquid (but no cooling), the temperature of MG7 is around 45 degrees, about 20 degrees higher than the other Mugast detectors. |
Fixed | e786s |
Wed Jun 26 07:04:06 2019 |
Freddy | CATS | General | N/A | Update of CATS calibrations |
New calibrations in :
/home/mugast/analysis/nptool/Projects/calibration/cats/CATS2_X.vamos2019_e786s.npt
/home/mugast/analysis/nptool/Projects/calibration/cats/CATS2_X.vamos2019_e786s.npt
Calibration.txt was modified accordingly.
Attached are the CATS positions for run 56 and 58 (after the central strip problem) |
Fixed | e793s |
Tue Mar 9 10:22:16 2021 |
mugast | DAQ | Hardware | N/A | U2M scaler configuration |
U2M
1-FAG
2-OR MM-MG
3-OR AGATA
4-TRIG VAMOS
5-CATS CLEAN
6-DT && OR MM-MG
7-100 Hz
8-100 Hz & DT
9-MUVI1
10-MUVI2
11-MUVI3
12-MUVI4
15-CATS2 direct
16- FINGER (unused) |
Fixed | e768s |
Sat Jul 20 19:21:56 2019 |
Marlene, Nicolas, Christian, Fairouz | OFFLINE | General | | Trying to understand AGATA g-ray yields |
goal: we want to check whether the yields of the 1297.7 keV (from 19Ne 1536, 3/2+, l=1 state) and 1340 keV (from 19Ne 1615, 3/2-, l=2 state) g-ray lines is compatible with what we expect from x-sec calculations
conditions: we consider runs 112, 115 and 116
observations:
N(1297) = 17 g-rays
N(1340) = 23 g-rays
remarks:
Given x-sec from mirror nucleus (Francois 15N(7Limt) paper) we expect N(1340) >~ N(1297)
ingredients:
1. beam normalization
We use the TAC_FPMW_HF as a proxy. During the same time we integrate the prompt peak and compare the integrated OR VAMOS scaler, we find Scaler(OR VAMOS)/N(TAC) = 193.
We use the comparison of the OR VAMOS (pps) and the beam profiler (pps), we find profiler/OR VAMOS = 1e4
We obtain (2.17e5 + 6.44e4 + 3.52e5)*193*1e4 = 1.2 e12 15O incident particles (at profiler position!)
2. target thickness -> known to be 1.25 mg/cm2 of LiF (RBS measurement)
N(Li) = 1.25e-3 / (19+7) * 6.02e23 at/cm2
3.efficiencies
AGATA @ 1.3 MeV -> 7.5 %
VAMOS intrinsic -> 67 % (Eff_Check.C macro applied to run 116)
MUGAST -> 50 % (lab, geometry), needed because MUGAST is the main trigger
4. 19Ne charge state
we assume 40 % for 9+
5. g-ray branching ratio -> taken from NNDC
6. cross-section
we calculate differential cross section for the 1536-keV 19Ne state (FRESCO, FR-DWBA)
-> at 0 deg, ds/dW =
-> integrated x-sec in VAMOS acceptance (4 deg (lab) -> 20 deg (cm)) = 445 micro barn (C2Sa = 1)
-> taking into account know spectroscopic factor form analog state -> 89 micro barn
Conclusion:
for the 1536-keV 19Ne state we obtain 30 g-rays, instead of 17.
Discussion:
This factor of two could be well within the mirror symmetry assumption. However it seems it is also the case for the 1615-keV 19Ne state, so would not it be a systematic error with a factor of two missing somewhere (beam transmission between the profiler and the target? deficiencies?)? |