MUST2 SAMURAI_2018 S3-LEB-LPC SUPERNEMO MUGAST EXPAND SCALP GALATRON HiCARI VELO
  MUGAST, Page 132 of 132  Not logged in MUGAST
Status ExpNbr Date Author Type Category Target-Source Subject
Fixede793s Wed Mar 17 13:58:29 2021 OttoTimeRUNGeneralN/ATimeCalibratorRun
*** Run Time Calibrator FSC ***
- Run: 644
- MUVI: MUVI1
- Side : MUFEE X (Junction)
- Telescope: 1, 2, 3, 4
Fixede793s Wed Mar 17 14:10:30 2021 OttoTimeRUNGeneralN/ATimeCalibratorRun
*** Run Time Calibrator FSC ***
- Run: 645
- MUVI: MUVI1
- Side : MUFEE Y (Ohmic)
- Telescope: 1, 2, 3, 4
Fixede793s Wed Mar 17 14:22:31 2021 OttoTimeRUNGeneralN/ATimeCalibratorRun
*** Run Time Calibrator FSC ***
- Run: 646
- MUVI: MUVI2
- Side : MUFEE X (Junction)
- Telescope: 1, 2, 3, 4
Fixede793s Wed Mar 17 14:34:43 2021 OttoTimeRUNGeneralN/ATimeCalibratorRun
*** Run Time Calibrator FSC ***
- Run: 647
- MUVI: MUVI2
- Side : MUFEE Y (Ohmic)
- Telescope: 1, 2, 3, 4
Fixede793s Wed Mar 17 14:46:59 2021 OttoTimeRUNGeneralN/ATimeCalibratorRun
*** Run Time Calibrator FSC ***
- Run: 648
- MUVI: MUVI3
- Side : MUFEE X (Junction)
- Telescope: 1, 2, 3, 4
Fixede793s Wed Mar 17 14:59:17 2021 OttoTimeRUNGeneralN/ATimeCalibratorRun
*** Run Time Calibrator FSC ***
- Run: 649
- MUVI: MUVI3
- Side : MUFEE Y (Ohmic)
- Telescope: 1, 2, 3, 4
Fixede793s Wed Mar 17 15:11:37 2021 OttoTimeRUNGeneralN/ATimeCalibratorRun
*** Run Time Calibrator FSC ***
- Run: 650
- MUVI: MUVI4
- Side : MUFEE X (Junction)
- Telescope: 1,
Ongoinge793s Wed Mar 17 15:17:39 2021 Emmanuel COFFLINEGeneral New gamma gamma analysis
The level scheme is based on coherent check of
1- gamma gamma
2- gamma gated by Ex
3- Ex gated by gamma
Attachment 1: 48K.pdf
48K.pdf
Fixede793s Wed Mar 17 15:20:08 2021 OttoTimeRUNGeneralN/ATimeCalibratorRun
*** Run Time Calibrator FSC ***
- Run: 651
- MUVI: MUVI4
- Side : MUFEE Y (Ohmic)
- Telescope: 1,
Fixede793s Wed Mar 17 19:19:05 2021 FrancoOFFLINEGeneralCD2Mugast detectors disaligned in Ex
The Ex distributions gated on the different MG detectors show large differences, up to 500 keV. In the attached figure I show as an example the comparison between two nearby detectors, MG3 and MG4.
I tried a rough alignment of the Ex by shifting it manually and setting the first main peak at Ex=0 (essentially taking MG5 as the reference, since his first peak is at 0).
These are the shifts applied:
MG1 -> -580 keV
MG2 -> -280 keV
MG3 -> -550 keV
MG4 -> -100 keV
MG5 -> 0 keV
MG7 -> -400 keV
The resulting Ex distribution is plotted in the second attachment, compared with the original below. The resolution of the first peak (assuming there's a single level there) is 420 keV FWHM.
I think it would be worth having the position of the MUGAST detectors re-measured.
Attachment 1: detectors_disalignment_Ex.png
detectors_disalignment_Ex.png
Attachment 2: Ex_aligned_vs_unaligned.png
Ex_aligned_vs_unaligned.png
Fixede793s Thu Mar 18 16:25:56 2021 Emmanuel COFFLINEGeneral Efficiency gamma AGATA --- real measurement run70

Emmanuel C wrote:
TF1 *fit_1 = new TF1("fit_1","TMath::Exp([0]+[1]*TMath::Log(x)+[2]*pow(TMath::Log(x),2.0)+[3]*pow(TMath::Log(x),3.0)+[4]*pow(TMath::Log(x),4.0))",10,5000); //NRJ traite en keV et efficiency en %


Data

40.000000 3.404000 0.070000
45.000000 6.512000 0.150000
121.782997 14.250000 0.300000
244.692001 11.880000 0.270000
295.938995 11.870000 0.500000
344.276001 11.170000 0.240000
411.114990 9.926000 0.330000
443.976013 11.050000 0.290000
778.903015 8.007000 0.180000
867.388000 7.562000 0.240000
964.130981 7.492000 0.180000
1085.800049 7.110000 0.160000
1112.115967 6.956000 0.150000
1212.949951 6.113000 0.190000
1408.010986 6.157000 0.130000


p0 -9.87216e+01
p1 6.98517e+01
p2 -1.78362e+01
p3 2.00526e+00
p4 -8.41808e-02
Fixede793s Fri Mar 19 09:54:58 2021 Adrien, Freddy and FrancoGRITGeneral3-alphaAlpha calibration and noise on MG3 and MG4 after the experiment
While starting the alpha source runs after the experiment we found unexpected noise on MG3 and MG4 which cannot be excluded just by masking some Y mates (The X mates were already masked for both of them). We cannot figure out the origin of this noise.

Run 652 and 653 -> alpha runs without pedestal suppression
Run 655 -> alpha run during the night with pedestal suppression. Here MG3 and MG4 are not in the trigger.
Run 658 -> alpha run after an attempt to mask some noisy strips. The number of ORD is anyway high (some 10^4) but we see some alphas on MG3 and MG4.
Run 660 -> same as 658 but with higher thresholds on X (8250) and Y (7600 on MG3 and 7950 on MG4) to write less on disk but actually nothing changes. Therefore we are writing about 2.7 GB per hour.

The other runs (654, 656, 657 and 659) can be discarded.
Fixede793s Mon Mar 22 16:35:46 2021 OttoRunRUNGeneralN/ARun67
*************************
Run : 67
*************************

Start at 2021-03-22 16:34:11.552975

run67. Time calibrator in TDC VAMOS

PERIOD: 80 ns

Trigger VAMOS


Raw Data: /data/mugastX/e793s/acquisition/run/run_0067.dat.22-03-21_16h34m11s
Raw RootFile: /home/mugast/Analysis_e793s/RootR/r0067_000r.root
Fixede793s Mon Mar 22 18:15:50 2021 mugastRUNGeneralN/ATACS calibration - run 662
TACS:

FAG-CATS2 (range 500 ns)
VAMOS-AGATA (range 500 ns)
CATS2-CATS2 (not in modular label) (range 500 ns)
AGATA-CATS2 (range 200 ns)

Time calibrator settings:

640 ns range
20 ns steps
Fixede793s Mon Mar 22 19:04:55 2021 mugastRUNGeneralN/ATACS calibration - run 653
TACS:

MUGAST-AGATA (range 2 us)
MUGAST-CATS2 (range 1 us)
MUGAST-CATS2b (range 2 us)
MUGAST-VAMOS (range 2 us)
VAMOS-CATS2 (range 2 us)

Time calibrator settings:

2.56 us range
80 ns steps
Fixede793s Tue Mar 23 10:22:48 2021 Emmanuel COFFLINEGeneral Efficiency gamma AGATA --- real measurement run70

I have been working on the high energy response.
The point is that we do not have source measurement beyond 2 MeV to constrain the fit.
In the attached file, the experimental points are the measured from run 70 in 152Eu source. The fit is then extrapolated up to high energy.
I have simulated the efficiency at 3.5 MeV in GEANT4 including real geometry, missing channels, unefficiency of capsules etc.... The overall agreement was checked on the 1408 line. The 3.5 MeV simulated point is shown. It disagrees strongly with the extrapolation. The blue fit includes the simulated point. It doesn't change the efficiency evaluation < 1.5 MeV but correct the high energy response.
Below, updated parameters

p0 -6.34543e+01
p1 4.24746e+01
p2 -1.00304e+01
p3 1.03468e+00
p4 -3.97076e-02


TF1 *fit_1 = new TF1("fit_1","TMath::Exp([0]+[1]*TMath::Log(x)+[2]*pow(TMath::Log(x),2.0)+[3]*pow(TMath::Log(x),3.0)+[4]*pow(TMath::Log(x),4.0))",10,5000); //NRJ traite en keV
Attachment 1: effi.png
effi.png

ELOG Home Page