MUST2 SAMURAI_2018 S3-LEB-LPC SUPERNEMO MUGAST EXPAND SCALP GALATRON HiCARI VELO
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Status ExpNbr Date Author Type Categorydown Target-Source Subject Text Attachments
Fixedcom2019 Sat Apr 6 08:18:55 2019 mugastRUNSoftwareCD2Online Scalers run 256 @8h00 am 06/04 for reference    Scalers060419-08am.pngMust2X060419-08am.pngMust2Y-060419_08am.pngMust2MugastXYMatrix060419_08am.pngMUGAST060419_08am.png 
Fixedcom2019 Sat Apr 6 10:57:35 2019 NicolasOFFLINESoftwareCD2time of flight v.s. energy in MUGAST (run 256, all stat)   ToF_dE_MUGAST_run256_all_stat.pdf 
Fixedcom2019 Sat Apr 6 11:40:08 2019 mugastOFFLINESoftwareCD2 AGATA spectrum in coincidence with MUGAST VAMOS run 256    04.png 
Fixedcom2019 Sun Apr 7 14:24:18 2019 ValerianOFFLINESoftwareCD2Ex and E gamma with all statistic (run 256+257)   bilan_run256_and_257_Ex_Egamma.png 
Fixedcom2019 Tue Apr 9 10:44:40 2019 ValerianMUST2SoftwareCD2CsI Calib files from the commissioning for protonCsI calibration obtained from the proton data
of the commissioning of mugast.
 Cal_CsI_E_MM1.calCal_CsI_E_MM2.calCal_CsI_E_MM3.calCal_CsI_E_MM4.cal 
Fixede744s Tue Apr 9 18:08:22 2019 Marlène and FrançoisDAQSoftware new inputs in the ADC Mugastnew inputs in the ADC mugast
T_Mugast_HF = input N°2
E_AGATA =  agata 42 = input N°3
  
Pinnede744s Wed Apr 10 11:57:37 2019 A. LemassonOFFLINESoftware VAMOS Conversion HowTo
[B]HOW TO convert a run in VAMOS[/B] 
[LIST]
  
Pinnede786s Wed Apr 10 13:30:48 2019 Valerian, Adrien and Antoine (edit by Louis)OFFLINESoftwareN/AHow to perform analysis for e786s[U][B]
Here is the updated procedure to convert
a run, with VAMOS data and add those data
  
Fixede744s Thu Apr 11 11:36:09 2019 ValerianOFFLINESoftwareCH2Comparison between the two e744Current calibration is off, a shift of -1.5MeV
was done to reproduce the previous data.
 current_exp_old_e744.png 
Fixede744s Thu Apr 11 13:43:26 2019 ValerianOFFLINESoftwareCH2Target position for 14N runs   XY_run14N.pngXshift_run14N.pngYshift_run14N.png 
Fixede744s Thu Apr 11 16:07:59 2019 Valerian and LouisOFFLINESoftwareCH2HF resolutionUsing 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
 T_CATS2_HFns.png 
Fixede744s Thu Apr 11 18:20:27 2019 Valerian and DiegoOFFLINESoftwareCH2Timing issue between vamos and mugastA cut is seen on the TAC between MUGAST and
the focal plane multiwire of VAMOS when one
select XF or DC0_Y>-1500
 T_MUGAST_FPMW.pngT_MUGAST_FPMW1.png 
Fixede744s Fri Apr 12 10:12:45 2019 ValerianOFFLINESoftwareCH2Comparison between HF and CATS for ELab ThetaLabUsing the HF show noises that is not seen
with CATS on the ToF spectra
 ELabThetaLabrun87_E744_HFvsCATS.png 
Fixede744s Fri Apr 12 14:13:11 2019 Giuseppe D'AgataOTHERSoftwareN/AConverted runs
Runs additionally converted up to now:
70
  
Fixede744s Fri Apr 12 19:44:09 2019 diegoVAMOSSoftware SetAlias script for VAMOS identification   SetAlias.C 
Fixede744s Fri Apr 12 22:44:43 2019 Valerian and DiegoOFFLINESoftwareCH213N measured in Vamos do correspond to protons events in MUST2Doing 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!!!
 Vamos13N_and_MUST2protons.png 
Fixede744s Sat Apr 13 00:27:08 2019 iulian nicolas Nikola MariluzRUNSoftwareCH2Screenshots run119 v1   21x 
Fixede744s Sat Apr 13 22:45:27 2019 Beyhan, Sylvain, JaromirAGATASoftwareN/AAgata yellow phase 1 minuteAgata yellow 1 minute

All the trigers emitted by (every) single
  
Fixede744s Sat Apr 13 23:19:57 2019 Valerian, Freddy, Iulian and FairouzOFFLINESoftwareCH2Very preliminary results for two protonsJoin are very preliminary spectra for the
two protons events gated on 13N in VAMOS
with a multiplicity 1 event in MUST2. This
 TwoProtonsMult1_run122_0_1.png 
Fixede744s Sun Apr 14 12:11:52 2019 Valerian and IulianOFFLINESoftwareCH2VERY VERY preliminary results Gamma-pAround 8-10 events are found in the good energy
vs Brho region and Si_T vs Si_E region for
the gamma emission.
 EPCM_Brho_gamma.pngPossiblePafterGamma_ToF.pngEpcm_gamma.png 

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