AIDA GELINA BRIKEN nToF CRIB ISOLDE CIRCE nTOFCapture DESPEC DTAS EDI_PSA 179Ta CARME StellarModelling DCF K40
  BRIKEN, Page 13 of 21  ELOG logo
Entry  Wed Mar 29 13:31:37 2017, J Agramunt, R. Caballero, T. Davinson, C. Griffin, O. Hall, D. Kahl, G. Kiss, J. Liu, S. Nishimura, V. Phong, JL Tain, Start of parasitic 170329_Conf_BrikenFull.xlsx
Start of parasitic Ca beam
(main experiment "New isotope search", Ahn et al.)
Entry  Thu Nov 3 05:46:48 2016, Iris, Ale, Background measurement 
Background measurement for threshold determination

Entry  Mon Jun 12 02:45:44 2017, Iris Dillmann AT, Setup detectors. Id of Ancillary@BRIKEN Setup-26May2017.pngOfflineConf_Signals.csv
Attachment 1: Setup detectors 
Attachment 2: example of configuration file (valid only for RIBF127). The Id of the ancillary detectors are:
Entry  Mon Nov 7 09:05:09 2016, Iris, Draft for Run sheet Run_sheet-Nov16-v2.pdfRun_sheet-Nov16-v2.docx
Attached is the draft for the paper run sheet (version 2). If something is missing, please let me know.
Entry  Wed Nov 9 01:02:53 2016, Iris, Elog 
From Nov. 9th on we use the Takechi ELOG for the run information:
http://ribf-exp.riken.jp/elog/RIBF123/ 
    Reply  Wed Nov 9 01:04:35 2016, Iris, Drawing of present setup Setup-161109-Takechi.pdf
This is the setup which was used for the Ni runs (from Nov. 8th evening on).

Note (Nov. 10th): Alejandro built a U-shaped Pb wall, the degrader inside AIDA was removed and possibly a Al plate was installed. This has to be checked
Entry  Wed Nov 9 02:02:22 2016, Iris, Boron rubber from India BPE2_Clr.jpgquotation_220213.pdfflex_boron_2871.pdf
The boron rubber from India is BR-2871, price US-$ 2700 for 2pc 1m x 2m x 3.3mm.
52% B content, density 1.61 g/cm3
Entry  Fri Mar 31 04:57:01 2017, ID,YS,JLT,OH, 40Mg run 35 
Date: 31/03/2017
Start: 12:24
BRIKEN run: 035
Entry  Sat Apr 1 06:49:00 2017, ID,GK,JA,DK,SN,JLT, 37Na run 58 
Date: 1/04/2017
Start:14:48
BRIKEN run: 58
Entry  Fri Mar 31 01:50:15 2017, ID, RCF, 40Mg Run 032 
Date: 31/03/2017
Start: 10:01
BRIKEN run: 032
Entry  Fri Mar 31 23:41:57 2017, ID, LIU, DK, GK, 37Na run 53 
Date: 1/04/2017
Start: 07:41
BRIKEN run: 53
Entry  Sat Apr 1 22:41:22 2017, ID, GK, SN, Liu YS JLT, 38Mg run 73 
Date: 2/04/2017 
Start: 06:37
BRIKEN run: 73
Entry  Fri Mar 31 01:01:58 2017, ID RCF OH, Run 031 
Date: 31/03/2017
Start: 08:58
BRIKEN run: 31
Entry  Fri Mar 31 02:26:19 2017, ID RCF, 40Mg Run 033 
Date: 31/03/2017
Start: 10:23
BRIKEN run: 033
Entry  Fri Mar 31 11:46:44 2017, ID PV CG, 40Mg Run 041 
Date: 31/03/2017
Start: 19:43
BRIKEN run: 41
Entry  Fri Mar 31 03:26:53 2017, ID OH SN, 40Mg Run 034 
Date: 31/03/2017
Start: 11:23
BRIKEN run: 034
Entry  Sat Apr 1 08:39:47 2017, ID OH JLT, 36Ne 37Na run 059 
Date: 1/04/2017
Start:16:38
BRIKEN run: 59
Entry  Fri Mar 31 03:54:26 2017, ID JLT, Run 034: gamma spectra background lines natural-gammas.pdf
There is a strong background line at ~1293 keV. According to the attached document this could come from the
neutron activation of 115In to 116In (14s halflife) of Indium seals.
Entry  Sun Apr 2 00:19:01 2017, ID JA GK CG YS SN Liu VP , 39Al run 74 
Date: 2/04/2017 
Start: 08:17
BRIKEN run: 74
Entry  Sun Apr 2 00:44:01 2017, ID JA GK CG VP Liu JLT, 39Al run 75 
Date: 2/04/2017 
Start: 08:42
BRIKEN run: 75
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