MUST2 SAMURAI_2018 S3-LEB-LPC SUPERNEMO MUGAST EXPAND SCALP GALATRON HiCARI VELO
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Fixed, e793s, Thu Mar 11 09:04:38 2021, adrien, ONLINE, General, CD2, Elastic scattering in MM5 run53_mm5_elastic.png
looking at E vs strip number in MM5 we see clearly the pp and dd elastic scattering.
Fixed, e793s, Thu Mar 11 12:11:16 2021, Freddy Adrien, OFFLINE, General, N/A, Elastic - Fixed MM5 position ELabThetaLabwithElastic.png
We roughly fixed the position of MM5 in the mugast.detector file.

Kinematic line for elastic channels are now clearly visible.
Fixed, TEST, Fri Mar 1 12:07:44 2019, Freddy, GRIT, General, 3-alpha, Efficiency reconstruction comparison.pdfcomparison.Calpha_eff.root
blue: reconstructed efficiency using alpha run 40 (arbitratily normalized)
red: simulated efficiency
    Fixed, e793s, Thu Mar 18 16:25:56 2021, Emmanuel C, OFFLINE, General, , Efficiency gamma AGATA --- real measurement run70 
[quote="Emmanuel C"] 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 %
    Fixed, e793s, Tue Mar 23 10:22:48 2021, Emmanuel C, OFFLINE, General, , Efficiency gamma AGATA --- real measurement run70 effi.png

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. 
Fixed, e793s, Sat Mar 13 18:37:01 2021, Emmanuel C, OFFLINE, General, , Efficiency gamma AGATA 
 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))",100,5000);
 //NRJ traite en keV et efficiency en %
     p0          -7.84071e+00   
Pinned, e793s, Tue Mar 9 09:35:18 2021, Adrien, OTHER, General, N/A, E793s proposal Proposal_K48_by_dp_MUGAST_FINAL.pdf
[SIZE=6][B]Attached is the proposal of the experiment.[/B][/SIZE]
Fixed, e744s, Mon Apr 8 08:30:50 2019, iulian, OTHER, General, N/A, E744s to-do list , proposal and other relevant documents Proposal__15F_v6.pdftime_request_E744.pdfe744s.pdf
To do list

[COLOR=blue]- ask  final beam energy for the 14O beam (include CATS removal)-> E=7.60 MeV/u  Done[/COLOR]
Fixed, e744s, Mon Apr 8 15:17:28 2019, François, TARGET, General, , E744 Targets  20190408_143035.jpg

Targets mounted on holder
Fixed, e744s, Wed Apr 10 11:46:04 2019, iulian, BEAM, Social, N/A, E744 Status 
Refrigeration problem, beam stopped.
Optimistic estimation: they need 1 UT to setup CIME => 14N could be back around 20h.
Optimistic scenario still on track 
Fixed, e744s, Fri Apr 12 13:34:33 2019, iulian, OTHER, General, N/A, E744 Status 
1) Beam tuning during the night.
2) around 04h00 started runs at 4e+4
3) beam intensity decreased to 1e+4 @7h30 in the morning.
Fixed, e768s, Thu Jul 18 11:52:59 2019, Marlène, OTHER, Hardware, N/A, Division of SQUARE & MUST2 

MUST2 DIV is now 10 (input 7 of GMT)
Fixed, e744s, Mon Apr 15 01:06:57 2019, Freddy, BEAM, General, N/A, Dipole trip 
A dipole tripped somewhere on the line, the operators put it back to value very quickly. Interruption of the beam for 2 minutes at 1h06.
Fixed, e786s, Fri Jun 28 09:56:59 2019, Bertrand, Valerian and Adrien, BEAM, General, N/A, Dipole stopped in the morning? 
Dipole restart at 10. Shoudl be checked with time stamp.
Fixed, e768s, Tue Jul 23 15:03:54 2019, Diego Ramos, OTHER, Hardware, N/A, Diamond threshold 
The threshold of the Diamond was increased from ~50 mV to ~300 mV
Fixed, e768s, Sun Jul 21 17:59:04 2019, Christian, VAMOS, Hardware, LiF, Diamond detector trigger level and rate dependency IMG_1065.JPGIMG_1064.JPG
The diamond detector has tended to increase in rate when it is hot (peaking late afternoon) and decreasing when it is cold (with a minimum just before sun-rise).
Some of the rate could therefore be temperature dependent noise levels rising above the trigger threshold.
Fixed, e768s, Tue Jul 23 04:31:34 2019, Jenn & Christian, BEAM, General, , Diamond Scaler screenshot diamondscaler_run126_3.png
 
Fixed, , Fri Jan 25 17:02:25 2019, Marlène, GRIT, General, , Detectors numbering MUGAST_detectors.pdf
 
Fixed, , Fri Feb 15 15:31:28 2019, Marlène, GRIT, General, N/A, Detectors bias 
 
Fixed, TEST, Thu Mar 12 10:14:02 2020, Marlène & Franco, GRIT, Hardware, N/A, Debugging the cooling system 
We realized that the increase of temperature of MG7 and MG9 during run 600 (alpha calibration) was due to the fact that a loop of the cooling system was
not working since the pipes were not properly connected. We re-connected them and switched on the low voltage without making the vacuum just to monitor
the evolution of the temperature.

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