MUST2 SAMURAI_2018 S3-LEB-LPC SUPERNEMO MUGAST EXPAND SCALP GALATRON HiCARI VELO
  MUST2, Page 5 of 48  Not logged in MUST2
Ongoing, e744, Thu May 24 02:30:52 2018, iulian, RUN, General, N/A, RUN 440 14N no target trigger Must & cats %100 run440.png
RUN 440 
14N beam  \
no target 
Ongoing, e744, Thu May 24 05:59:44 2018, iulian, MUST2, General, N/A, run 444 t1-t4 trigger no target 14n beam mm5_8_run445.pngmm5_7_run444.pngmm5_6_run444.pngmm5_5_run444.pngmm5_4_run444.png
run 444 
t1-t4 trigger
 no target 
Ongoing, e744, Thu May 24 06:30:27 2018, iulian, RUN, General, N/A, run 445 t1-t4 trigger no target 14n beam no CATS mm5_run445_3.pngmm5_run445_2.pngmm5_run445_1.png
 
Ongoing, e744, Fri May 25 02:57:44 2018, Valerian and Iulian, OFFLINE, General, CH2, Simulation Azure 1H(14N,p) and measurement  o15.pdfE_cm_ThetaLab_0_4.pdfE_cm_ThetaLab_2_3.pdfE_cm_ThetaLab_10_12.pdfE_cm_ThetaLab_15_20.pdf
We can know conclude without any doubt that we were able to measure resonances from 1H(14N,p)14N. The resolution with a rough analysis and the current bad
calibration is around 180keV in the com.
Identification of resonances is still difficult but some structure seems consistent with previous works. Also, at higher energy there are only few measurement
Ongoing, e744, Fri May 25 15:10:23 2018, François, CATS, Hardware, , delay on CATS 
CATS delay 500 ns was changed to 300 ns, in order to get the stop signal on MUST2 TAC well within the range of the TAC. 
Ongoing, e744, Fri May 25 15:19:38 2018, Cristina, OFFLINE, General, , isomers present in the 14N runs 14Nruns_isomers_EXL.pdf14Nruns_isomers_PPT.pdf

Attached are some pictures of the energy_vs_time spectra for EXL and PPT detectors recorded during 14N runs
Ongoing, e744, Fri May 25 16:49:53 2018, e748, MUST2, General, CH2, Raw dE-TOF bidim for the 5 telescopes zith the 14N beam Example1.png
Pedestal seems not to be aligned for T4
Ongoing, e744, Fri May 25 23:15:57 2018, Valerian, OFFLINE, General, CH2, Oxygen 15 excitation function Exc_15O.pdf
After a quick analysis, we can conclude that MUST2 is working for resonant elastic scattering. We find a resolution of 125 keV which will improve with a
better analysis, as we are using a basic calibration for CsI Energy.
Ongoing, e744, Sat May 26 03:23:46 2018, Valerian, OFFLINE, General, CH2, 15O excitation function as a function of ThetaLab Ex_15O.pdf
 
Ongoing, e744, Sat May 26 05:02:42 2018, Valerian, TARGET, General, CH2, Problem with the target for run 2004 and 2010 Target_Issue_2004_2010.pngtargets.jpg
The target seems identical between the two runs... We will have to investigate to understand what is going on.

The decision is to change the target 5 for the target 4 104um from georges.
Ongoing, e744, Sat May 26 07:03:12 2018, Valerian and Iulian and Francois, OFFLINE, General, CH2, First picture for 15F from runs 2010-2013 Ex_15F_proj_0_8deg_17_27.pdfsig_theo.jpg
Target -> Thick target (Sandwich target ??)

The predictions are different....  
Ongoing, e744, Sat May 26 07:32:17 2018, Valerian, pedja, mihai, RUN, General, CH2, Run 2015 after vacuum problem of Css1 target 4 Scalers_start_run2015.png
[U][B]Run 2015[/B][/U] 
26/05/18
start @7h29
Ongoing, e744, Sat May 26 10:06:06 2018, Giuseppe, Dieter, RUN, General, CH2, Run 2018 Scalers_start_run2018.pngScalers_stop_run2018.pngMM_IMPACT_stop_run2018.png
Run 2018 
Start @ 09:56 26/05/2018
Stop @ 10:51
Ongoing, e744, Sat May 26 20:20:55 2018, Valerian, OFFLINE, General, CH2, 15F observations for target 4 (100um) Ecm_Thetacm_target4_notes.pdfEx_15F_proj_0_4deg_Ecm_target4.pdfEx_0to40degEcm_15F.pdf
Analysis offline permits us to conclude that the current target has the good size to observe our resonances.
Ongoing, e744, Sat May 26 20:23:52 2018, Cristina Iulian, OFFLINE, General, , PPT gamma spectrum runs_target4_proton_prompt_PPT.pdf
 Attached is the gamma spectrum from PPT detector with a condition on prompt (T_MM_PPT), proton detected in MUST and multiplicity event equal to 1
Ongoing, e744, Mon May 28 02:07:41 2018, Valerian, OFFLINE, General, CH2, New improved resolution for 14N et 15F Exc_15O_newpos.pdfExc_15F_newpos.pdf
After correcting position for the Must2 detectors by taking into account the real hit position on the target that was (0,15cm,0) and not (0,0,0). The way
to do it was to artificially move every detector 15cm lower.
Ongoing, e744, Mon May 28 20:28:50 2018, Valerian and Simon, OFFLINE, General, CH2, Explanation for the 0 degree low energy proton explanation_spotT5.pdf
The 0 degree energy proton are coming from the beam hitting the aluminum target. If you do a cut on the beam projection on T5 you obtain the black dot on
the joined plot.
Ongoing, e744, Mon May 28 23:14:26 2018, Valerian and Iulian and Phil, OFFLINE, General, CH2, New hint of the 5/2- resonance New_resonance_hint.pdf
We see a new hint of a resonance
Ongoing, e744, Tue May 29 00:17:18 2018, Night shifter, BEAM, General, Carbon, Beam intensity variation hv_run2103.png
Beam shut down at 00h03. Increase the intensity progressively up to now 00h18.
At 0:28: primary intensity dropped down to 0.
Ongoing, e744, Tue May 29 01:25:07 2018, Phil, Valerian, Franck, EXL-PPT, General, N/A, LaBr3 Background for reference Response-of-3-3-CeBr-3-and-LaBr-3-Ce-to-natural-background-radiation-Events-due-to.jpg.png
For reference, we include a picture of the LaBr3 background found by some random Google searching until we found a nice happy looking picture.

Remember (I'd forgotten despite having literally had this conversation with someone in the past) that the LaBr3 internal background lies at exactly the

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