MUST2 SAMURAI_2018 S3-LEB-LPC SUPERNEMO MUGAST EXPAND SCALP GALATRON HiCARI VELO
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New entries since:Thu Jan 1 01:00:00 1970
Status ExpNbr Date Author Type Category Target-Source Subject Text Attachments
Ongoinge744 Mon May 28 23:14:26 2018 Valerian and Iulian and PhilOFFLINEGeneralCH2New hint of the 5/2- resonanceWe see a new hint of a resonance  New_resonance_hint.pdf 
Fixede744 Mon May 28 23:52:19 2018 Simon and Louis (start), Franck (stop)RUNGeneralCarbonRUN 2103 DATA target 1 Carbonrun #2103
start @23h49
stop @1h51
 Scaler_start_Run2103.pngScaler_stop_Run2103.png 
Ongoinge744 Tue May 29 00:17:18 2018 Night shifterBEAMGeneralCarbonBeam intensity variationBeam shut down at 00h03. Increase the intensity
progressively up to now 00h18.
At 0:28: primary intensity dropped down to
 hv_run2103.png 
Fixede744 Tue May 29 01:08:22 2018 e748BEAMGeneralCarbonBeam intensityAt 0:46 primary beam intensity reaches 5 uA
-> 1.5e5 pps on CATS.
  
Ongoinge744 Tue May 29 01:25:07 2018 Phil, Valerian, FranckEXL-PPTGeneralN/ALaBr3 Background for referenceFor reference, we include a picture of the
LaBr3 background found by some random Google
searching until we found a nice happy looking
 Response-of-3-3-CeBr-3-and-LaBr-3-Ce-to-natural-background-radiation-Events-due-to.jpg.png 
Ongoinge744 Tue May 29 01:33:58 2018 Phil, Valerian, FranckEXL-PPTGeneral Gamma-ray spectra from PPTAttached are plots of gamma-ray energy spectra
from PPT.
 PPTSpectrum2D.pngPPTSpectrumPromptPeak1.pngPPTSpectrumPromptPeak2.png 
Fixede744 Tue May 29 02:01:58 2018 Franck, Valerian, PhilRUNGeneralCarbonRun 2104 - Target 1 CarbonRun 2104
Beam: 14O
Start @ 2:00  29 May 2018
 Scaler_start_Run2104.pngScaler_stop_Run2104.png 
Fixede744 Tue May 29 02:38:21 2018 Franck, Valerian, PhilONLINEGeneralCarbonSpectra and HV Start Run 2104   11x 
Fixede744 Tue May 29 04:08:52 2018 Franck, Valerian, PhilRUNGeneralCarbonRun 2105 - Target 1 CarbonRun 2105

Beam 14O
 Scaler_start_Run2105.pngScaler_stop_Run2105.png 
Ongoinge744 Tue May 29 05:07:33 2018 ValerianOFFLINEGeneralCH2Fusion evaporation background and physics dataComparison between the fusion evaporation
background and the data for the telescope
5 ~0degree angles and rough subtraction of
 Ex_15F_and_Carbon.pdfrough_backgrund_suppresion.pdf 
Ongoinge744 Tue May 29 05:24:34 2018 ValerianEXL-PPTGeneralCH2Comparison of background and physics data for gamma ray detectorsGamma ray spectrum for both targets seem extremely
close. Subtraction is then made but no gamma
show. More statistic is needed
 gamma_comparison_CH2_and_Carbon.pdfbackground_substr_gamma_ray.pdf 
Ongoinge744 Tue May 29 06:09:58 2018 Franck, PhilRUNGeneralCarbonRun 2106 - Target 1 CarbonRun 2106

Beam 14O (CATS: 1.4e5 pps)
 Scaler_start_Run2106.pngScaler_stop_Run2106.png 
Ongoinge744 Tue May 29 07:39:53 2018 Franck, PhilRUNGeneralCarbonRun 2107 - Restart after Reboot of VXI - Same problemLow FAG rate: 30 /s
Low ORD rates: 0-10 /s, 15 /s on MM5
  
Ongoinge744 Tue May 29 08:09:02 2018 e748RUNGeneralCarbonRUN 2108 - Target1 Carbon[B][U]Run 2019[/U][/B]

Acq recovered
 11x 
Ongoinge744 Tue May 29 08:59:18 2018 Freddy, Iulian, PierreRUNGeneralCH2Run 2109 - Target 4 CH2 - Tuning run[U][B]Run 2109[/B][/U]

Beam: 14O (1.5*10^5 pps)
 impact_Run2109_end.png 
Pinnede744 Tue May 29 09:30:42 2018 Freddy, Iulian, PierreRUNGeneralCH2Run 2110 - Target 4 CH2Run 2110

Beam: 14O (1.5*10^5 pps)
 Scaler_start_Run2110.pngimpact_Run2110.png 
Pinnede744 Tue May 29 09:54:01 2018 Freddy, Iulian, PierreRUNGeneralCH2Run 2111 - Target 4 CH2Run 2111

Beam: 14O (1.5*10^5 pps)
 8x 
Fixede744 Tue May 29 10:42:00 2018 FrancoisBEAMGeneral effective beam timeIn total, there were:

1.4 UT of 14O, average 2x10^5 pps
 os1.jpeg 
Fixede744 Tue May 29 12:06:05 2018 iulian maurycyOFFLINEGeneralCH2Carbon substraction The scale factor for Carbon subtraction is
1.224. This means: RealCountsHidrogen=Counts
CH2 - 1.224 * CountsCarbon 
 Carbon_runs_scale_factor.pdf 
Ongoinge744 Tue May 29 15:53:17 2018 Iulian MaurycyOFFLINEGeneralCH2 Angular distribution per telescope 1-4Angular distribution per telescope 1-4  ang_dist.pdf 

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