MUST2 SAMURAI_2018 S3-LEB-LPC SUPERNEMO MUGAST EXPAND SCALP GALATRON HiCARI VELO
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Fixed, e755, Mon Jul 2 18:51:11 2018, Pierre, RUN, General, Cryo-LH2, Run 232 31x
start: 18h49
stop: 20h41
Fixed, e738, Sun Jul 8 01:24:16 2018, Pierre, RUN, General, Cryo-LH2, Run 284 scaler_2018-07-08_01h25m36s.pngvisu_2018-07-08_01h26m12s.pngscaler_2018-07-08_03h10m42s.png
start: 1h15 
stop: 3h11
Fixed, e738, Sun Jul 8 03:13:35 2018, Pierre, RUN, General, Cryo-LH2, Run 285 scaler_2018-07-08_03h13m06s.pngvisu_2018-07-08_03h19m50s.pngvisu_2018-07-08_03h19m13s.pngvisu_2018-07-08_03h19m27s.pngvisu_2018-07-08_03h20m19s.png
start: 03h12
stop: 05h10
Fixed, e738, Sun Jul 8 05:09:11 2018, Pierre, RUN, General, Cryo-LH2, Run 286 13x
start: 05h11
stop: 07h00
Fixed, e738, Sun Jul 8 07:00:46 2018, Pierre, RUN, General, Cryo-LH2, Run 287 8x
start: 07h01
stop: 08h55
Fixed, e738, Mon Jul 9 07:55:05 2018, Pierre, RUN, General, Cryo-LH2, Run 302 scaler_2018-07-09_07h57m43s.pngvisu_2018-07-09_07h59m57s.pngvisu_2018-07-09_08h00m04s.pngvisu_2018-07-09_08h04m11s.png
start: 07h53
stop: 08h19
Fixed, e738, Fri Jul 13 00:45:45 2018, Pierre, RUN, General, Cryo-LH2, Run 367 
start: 00h44
Fixed, e738, Fri Jul 13 00:47:23 2018, Pierre, RUN, General, Cryo-LH2, Run 367 scaler_2018-07-13_00h46m09s.pngvisu_2018-07-13_00h51m01s.pngvisu_2018-07-13_00h50m40s.png
RUN 367

start: 00h44
Fixed, e738, Fri Jul 13 02:45:44 2018, Pierre, RUN, General, Cryo-LH2, Run 368 7x
RUN 368

start: 02h44
Fixed, e738, Fri Jul 13 04:48:19 2018, Pierre, RUN, General, Cryo-LH2, Run 369 7x
RUN 369

start: 04h47
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, Wed May 30 13:25:57 2018, Phil, Freddy, RUN, General, CH2, Run 2020 - target number 4 Scalers_start_run2020.pngRun2020_leakages_13h35.png
Run 2020

Start: 13h24m
Ongoing, e744, Wed May 30 13:48:02 2018, Phil, DAQ, General, N/A, Pulser values 
Here's a list of pulser values taken from the last few runs as a reference for what rate the "100-Hz" pulser is actually seeing.

All rates in Hz.
Fixed, e738, Fri Jul 13 09:35:26 2018, Olivier, Serge, Jacques, J-C, thomas, shumpei, daisuke, RUN, General, Cryo-empty, RUN 370 visu_2018-07-13_09h36m18s.pngscaler_2018-07-13_09h36m16s.png
Empty target + 9C. 
9h29 The beam is back. start 9h28 stop 11h21
e748 Exxx 2,1G 13 juil. 11:21 /data/e748X/e755/acquisition/run/run_0370.dat.13-07-18_09h28m21s
Ongoing, e755, Sat Jun 23 19:10:23 2018, Nori, OFFLINE, General, Cryo-LH2,  
 
Fixed, e755, Sat Jun 23 19:23:19 2018, Nori, OFFLINE, General, Cryo-LH2, 40Ca(p,d) analysis 7x
Analysis of run0072 (two hours accumulation).

Attachment 1:
    Fixed, e755, Sat Jun 23 20:07:49 2018, Nori, OFFLINE, General, Cryo-LH2, 40Ca(p,d) analysis 
Order-of-magnitude estimate of the target thickness.

We have about 5000 counts of 40Ca(p,d)39Ca(g.s.) in an angular range of 10-30 degrees.
    Fixed, e755, Mon Jun 25 17:28:03 2018, Nori, TARGET, Hardware, Cryo-LH2, Liquid hydrogen target logger screenshot_2018-06-25_17.20.41.pngscreenshot_2018-06-25_20.56.47.png
There was a sudden increase of the temperature at 4pm. Fortunately the cell is still filled with liquid.
Fixed, e755, Mon Jun 25 23:17:56 2018, Nori, MUST2, General, Cryo-LH2, DSSD multiplicity run0128_simult.pngrun0128_allstripsfired.pngAll_strip_fired.png
Data analysis of run0128 (38Ca physics run). The multiplicity distribution of DSSD x-strips is shown in
Attachment 1. The second peak centered at around 128, which is the number of strips of one detector, corresponds
to events where beam-like heavy ions are hitting the detector.

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