MUST2 SAMURAI_2018 S3-LEB-LPC SUPERNEMO MUGAST EXPAND SCALP GALATRON HiCARI VELO
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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
Ongoing, e744, Tue May 29 01:33:58 2018, Phil, Valerian, Franck, EXL-PPT, General, , Gamma-ray spectra from PPT PPTSpectrum2D.pngPPTSpectrumPromptPeak1.pngPPTSpectrumPromptPeak2.png
Attached are plots of gamma-ray energy spectra from PPT.

2-D plot is the PPT-CATS time (from PPT-MUST2 and MUST2-CATS time, obviously).
Fixed, e744, Tue May 29 02:01:58 2018, Franck, Valerian, Phil, RUN, General, Carbon, Run 2104 - Target 1 Carbon Scaler_start_Run2104.pngScaler_stop_Run2104.png
Run 2104
Beam: 14O
Start @ 2:00  29 May 2018
Fixed, e744, Tue May 29 02:38:21 2018, Franck, Valerian, Phil, ONLINE, General, Carbon, Spectra and HV Start Run 2104 11x
 
Fixed, e744, Tue May 29 04:08:52 2018, Franck, Valerian, Phil, RUN, General, Carbon, Run 2105 - Target 1 Carbon Scaler_start_Run2105.pngScaler_stop_Run2105.png
Run 2105

Beam 14O
Ongoing, e744, Tue May 29 05:07:33 2018, Valerian, OFFLINE, General, CH2, Fusion evaporation background and physics data Ex_15F_and_Carbon.pdfrough_backgrund_suppresion.pdf
Comparison between the fusion evaporation background and the data for the telescope 5 ~0degree angles and rough subtraction of this background.
Ongoing, e744, Tue May 29 05:24:34 2018, Valerian, EXL-PPT, General, CH2, Comparison of background and physics data for gamma ray detectors gamma_comparison_CH2_and_Carbon.pdfbackground_substr_gamma_ray.pdf
Gamma ray spectrum for both targets seem extremely close. Subtraction is then made but no gamma show. More statistic is needed
Ongoing, e744, Tue May 29 06:09:58 2018, Franck, Phil, RUN, General, Carbon, Run 2106 - Target 1 Carbon Scaler_start_Run2106.pngScaler_stop_Run2106.png
Run 2106

Beam 14O (CATS: 1.4e5 pps)
Ongoing, e744, Tue May 29 07:39:53 2018, Franck, Phil, RUN, General, Carbon, Run 2107 - Restart after Reboot of VXI - Same problem 
Low FAG rate: 30 /s
Low ORD rates: 0-10 /s, 15 /s on MM5
Ongoing, e744, Tue May 29 08:09:02 2018, e748, RUN, General, Carbon, RUN 2108 - Target1 Carbon 11x
[B][U]Run 2019[/U][/B]

Acq recovered
Ongoing, e744, Tue May 29 08:59:18 2018, Freddy, Iulian, Pierre, RUN, General, CH2, Run 2109 - Target 4 CH2 - Tuning run impact_Run2109_end.png
[U][B]Run 2109[/B][/U]

Beam: 14O (1.5*10^5 pps)
Pinned, e744, Tue May 29 09:30:42 2018, Freddy, Iulian, Pierre, RUN, General, CH2, Run 2110 - Target 4 CH2 Scaler_start_Run2110.pngimpact_Run2110.png
Run 2110

Beam: 14O (1.5*10^5 pps)
Pinned, e744, Tue May 29 09:54:01 2018, Freddy, Iulian, Pierre, RUN, General, CH2, Run 2111 - Target 4 CH2 8x
Run 2111

Beam: 14O (1.5*10^5 pps)
Fixed, e744, Tue May 29 10:42:00 2018, Francois, BEAM, General, , effective beam time os1.jpeg
In total, there were:

1.4 UT of 14O, average 2x10^5 pps
Fixed, e744, Tue May 29 12:06:05 2018, iulian maurycy, OFFLINE, General, CH2, Carbon substraction  Carbon_runs_scale_factor.pdf
The scale factor for Carbon subtraction is 1.224. This means: RealCountsHidrogen=Counts CH2 - 1.224 * CountsCarbon 

runs considered for the CH2 target
Ongoing, e744, Tue May 29 15:53:17 2018, Iulian Maurycy, OFFLINE, General, CH2, Angular distribution per telescope 1-4 ang_dist.pdf
Angular distribution per telescope 1-4
Ongoing, e744, Tue May 29 16:23:56 2018, Valerian Iulian Maurycy, OFFLINE, General, CH2, Hint of a 2p peaks  Two_proton_14Ovs12C.pdf
 
Fixed, e744, Tue May 29 17:14:41 2018, François, Freddy, Valérie, BEAM, General, , Beam back in D6 HV_MUST2_29mayAt17h20.pngHV_EXL_29mayAt17h21.png
At 17pm Tuesday 29th we have beam coming back in D6. Run (without storage)
NB: The current on T4 (with Hv set 60V) is fluctuating between 4 and 6.5 µA.
Ongoing, e744, Tue May 29 18:49:21 2018, Valerian, OFFLINE, General, CH2, Comparison of gamma prompt spectrum for EXL and PPT prompt_energyEXL_12C_14O.pdfprompt_energyPPT_12C_14O.pdf
Quick note, there is less data seen in EXL prompt. This should be investigated
Fixed, e744, Tue May 29 19:03:38 2018, Valérie (edit), RUN, General, CH2, Run #2112 BEAM BACK 14x
run #2112
Beam back given by the machine. 
Beam+ Lise team: Omar K and Pierre Delahaye, Jean-Charles T.

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