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Thu Nov 22 07:01:36 2018, AT, PID high mass seting (165Pm) - RIBF148  PID plot for the high mass setting (165Pm), run 2018, rare earth peak experiment. Partial statistics (~30h) from identification at F7. Please use for internal reports about the BRIKEN activities.   Tue Nov 6 21:51:54 2018, NT Brewer, New D4Off.conf for HV also on github  V A V/s V/s 1/0 ------ --------------- --------- ----- ---- ------- ------- ------ ------ ------------- 0 192.168.13.239 0 0 PA1 1450 0.0001 50 10 1 0 192.168.13.239 1   Mon Nov 5 22:47:40 2018, AT, JR, FM, PA, Low threshold, 252Cf, z=0cm, perpendicular 0 deg  252Cf at z=0cm, i.e 0 cm from the center of the detector,  source axis perpendicular at 0 deg  Low threshold.   Mon Nov 5 21:24:20 2018, AT, JR, FM, PA, Low threshold, 252Cf, z=25cm, perpendicular 90 deg  252Cf at z=25cm, i.e 25 cm from the center of the detector,  source axis perpendicular at 90 deg  Low threshold.   Mon Nov 5 19:55:20 2018, AT, JR, FM, PA, Low threshold, 252Cf, z=0cm, perpendicular 90 deg  252Cf at z=0cm, i.e 0 cm from the center of the detector,  source axis perpendicular at 90 deg  Low threshold.   Mon Nov 5 09:59:36 2018, MW, KR, suspicious clover G7 temp sensor  We observed 6 pm LN2 filling of both clovers on Monday Nov 5th. D4 went full within reasonable time of below 10 minutes. Filling of G7 was stopped by "emergency sensor" after about 15 minutes of filling.       Mon Nov 5 18:52:54 2018, MW, KR, suspicious clover G7 temp sensor    Quote: We observed 6 pm LN2 filling of both clovers on Monday Nov 5th.   Mon Nov 5 18:05:48 2018, AT, JR, FM, PA, Low threshold, 252Cf, z=25cm, perpendicular 0 deg  252Cf at z=25cm, i.e 25 cm from the center of the detector,  source axis perpendicular   Low threshold.   Mon Nov 5 16:43:43 2018, FM, PA,, Low threshold, 252Cf, z=25cm, Parallel downstream  252Cf at z=25cm, i.e 25 cm from the center of the detector,  source axis parallel downstream  Low threshold.   Mon Nov 5 15:10:43 2018, FM, PA,, Low threshold, 252Cf, z=15cm, Parallel downstream  252Cf at z=15cm, i.e 15 cm from the center of the detector,  source axis parallel downstream  Low threshold.   Mon Nov 5 13:43:57 2018, FM, PA, Low threshold, 252Cf, z=0cm, Parallel downstream  252Cf at z=0cm,ie center of moderator, source axis parallel downstream  Low threshold.   Mon Nov 5 12:04:08 2018, FM, PA, AT, Low threshold, 252Cf, z=15cm, Perpendicular 0deg  252Cf at z=15cm,ie center of moderator, source axis perpendicular at 0deg (typical orientation) Low threshold.   Mon Nov 5 09:32:00 2018, FM, JR, PA, AT, Low threshold, 252Cf, z=0cm, Perpendicular 0deg  252Cf at z=0cm,ie center of moderator, source axis perpendicular at 0deg (typical orientation) Low threshold.   Mon Nov 5 06:46:30 2018, KR, YR, MW, JLT, ..., Clover check  With detectors still on the floor we check signals and found that D4 gives no signal with PA power.  Two power supplies/cables were checked.   Fri Nov 2 14:18:54 2018, JLT, 136Sn at ZDS  Measurement of neutron background while Jungclaus experiment is running Secondary beam 136Sn at ~140MeV/u, Be target, 136Sn in the ZDS   Fri Nov 2 01:07:21 2018, JLT, 134Sn/133In on ZDS  Measurement of neutron background while Jungclaus experiment is running Secondary beam:    Wed Oct 31 03:41:33 2018, JLT, 134Sn at ZDS  Measurement of neutron background while Jungclaus experiment is running Secondary beam 134Sn at ~140MeV/u, Au target, 134Sn in the ZDS   Wed Oct 31 00:36:34 2018, JLT, 133In at ZDS  Measurement of neutron background while Jungclaus experiment is running Secondary beam 134Sn at XXMeV, Be target, 133In i the ZDS   Tue Oct 30 01:01:42 2018, JLT, AA, Adjustment of 3He thresholds  Background with BigRIPS+ZD already working No pulser   Mon Oct 29 12:08:12 2018, JR, JA, AT, Background  Background was measurement Pulser: NO   Sun Oct 28 07:41:03 2018, AT, JA, AA, Background  Dacq was reinitialized Background was measurement Pulser: YES   Fri Oct 26 15:15:55 2018, JA, ATS, ATD, JLT, AA, Background measurements  No pulser (inhibit in clock) DLT: 181026_2244_Bkg_NoPulser_114.dlt   Fri Oct 26 03:57:37 2018, ATS & JLT, Background  Background BRIKEN control measurement No DLT   Fri Oct 26 03:31:33 2018, AT2 & JA, Test pulser effect on baseline 6x We have tested possible change of the baseline in the digitizer due to the pulser connection. NO EFFECT has been found!   Fri Oct 26 03:24:25 2018, ATS & JLT, Background  Background BRIKEN control measurement No DLT   Thu Oct 25 16:08:53 2018, ATS & JLT, Lead bricks  Lead bricks in BRIKEN hole to protect AIDA   Thu Oct 25 16:04:17 2018, ATS & JLT, Background  Background BRIKEN control measurement No DLT   Thu Oct 25 09:32:25 2018, AT & AT, Low threshold, 252Cf, z=25cm, Perpendicular 90deg  252Cf at z=25cm,ie 25 cm upstream the beam, source axis perpendicular at 90deg with respect to typical orientation. Low threshold.   Thu Oct 25 09:18:24 2018, ATS & JLT, F11 plastic  F11 plastic (long plastic after MUSIC chamber)  connected to DACQ. The connections were re-cabled and verified.   Thu Oct 25 09:07:00 2018, ATS & JLT, BRIKEN Calibration check  We put the 252Cf source and check the aligment of 3He tubes gains: File: 181025_1600_252Cf_gaincheck.root   Thu Oct 25 04:14:00 2018, AT & AT, Low threshold, 252Cf, z=25cm, Perpendicular 90deg  252Cf at z=25cm,ie 25 cm upstream the beam, source axis perpendicular at 90deg with respect to typical orientation. Low threshold.   Thu Oct 25 00:53:43 2018, AT & AT, Low threshold, 252Cf, z=-25cm, Perpendicular 90deg  252Cf at z=-25cm,ie 25 cm downstream the beam, source axis perpendicular at 90deg with respect to typical orientation. Low threshold.   Wed Oct 24 16:11:32 2018, AT & AT, Low threshold, 252Cf, z=-25cm  252Cf at z=-25cm,ie 25 cm downstream the beam, source axis parallel. Low threshold.   Wed Oct 24 11:28:42 2018, AT & AT, Low threshold, 252Cf, z=-25cm  252Cf at z=-25cm,ie 25 cm downstream, source axis perpendicular, typical orientation. Low threshold.   Wed Oct 24 11:27:51 2018, AT & AT, Low threshold, 252Cf, z=10cm, source axis parallel  252Cf at z=10cm, source axis parallel upstream to the beam. Low threshold.   Wed Oct 24 07:42:42 2018, AT & AT, Low threshold, 252Cf, z=10cm, source axis parallel  252Cf at z=10cm, source axis parallel upstream to the beam. Low threshold.   Wed Oct 24 03:49:01 2018, AT & AT, Low threshold, 252Cf, z=0cm  252Cf at z=10cm, source axis perpendicular to beam axis, typical orientation. Low threshold.   Mon Oct 22 16:54:10 2018, AT & AT, background, low threshold, No Pulser  18/10/23 START: 00:53 18/10/24 STOP: 10:12  Background measurements. Checking noise!   Mon Oct 22 11:42:50 2018, AT & AT, 252Cf, z=25cm, no clovers  252Cf source placed using cardboard piece at z=25cm, source axis parallel upstream to the beam axis. 18/10/22 START: 19:44   Mon Oct 22 08:15:52 2018, AT & AT, 252Cf, z=15cm, no clovers  252Cf source placed using cardboard piece at z=15cm, source axis parallel to the beam axis. 18/10/22 START: 16:15   Mon Oct 22 03:11:32 2018, AT & AT, background, high threshold, Pulser UPC  18/10/22 START: 11:13 18/10/22 STOP: 15:59 Background measurements. Checking noise!   Sun Oct 21 15:16:40 2018, AT & AT, background, high threshold, Pulser RIKEN+ORNL  18/10/21 START: 23:16 18/10/22 STOP: 11:06 Background measurements. Checking noise!   Sun Oct 21 11:18:31 2018, AT & AT, Low threshold, NO pulser, 252Cf, z=0cm  18/10/21 START: 19:21 18/10/21 STOP: 23:04 252Cf at z=0cm, source axis perpendicular to beam axis, typical orientation.   Sun Oct 21 08:58:23 2018, AT & AT, background, high threshold, NO pulser  18/10/21 START: 16:58 18/10/21 STOP: 19:09 Background measurements. Checking noise!   Sun Oct 21 06:04:43 2018, AT & AT, background, high threshold  18/10/21 START: 14:10 18/10/21 STOP: 16:41 Background measurements. Checking noise!   Sun Oct 21 03:19:54 2018, AT & AT, background, high threshold  18/10/20 START: 20:30 approx  18/10/21 STOP: 11:20   Fri Oct 19 15:38:11 2018, AT & AT, 252Cf, z=0cm, no clovers, noise check individual tubes  18/10/19 START: 23:39 18/10/20 STOP: 18:30   Fri Oct 19 11:45:12 2018, AT & AT, 252Cf, z=0cm, no clovers  18/10/19 START: 19:46 18/10/19 STOP: 23:33   Fri Oct 19 11:28:31 2018, AT & AT, 252Cf, z=0cm, no clovers, test online dead time  During previous measurement a high dead time in the online was observed (50%). after restarting the crates and the GASIFIC70, we resume the measurement. The conf file is    Fri Oct 19 10:27:22 2018, AT & AT, 252Cf, z=0cm, no clovers (***** CHECK DATA)  18/10/19 START: 18:25 18/10/19 STOP: 19:19   Fri Oct 19 04:02:36 2018, AT & AT, 252Cf, z=0cm, no clovers (***** CHECK DATA)  18/10/19 START: 12:05 18/10/19 STOP: 16:44   Fri Oct 19 00:28:48 2018, AT2, JLT, SN, background measurement, no clovers  18/10/19 START: 08:31 18/10/19 STOP: 10:50   Thu Oct 18 15:24:40 2018, AT2, JLT, SN, 252Cf long measure, z=25cm beam upstream, no clovers  18/10/18 START: 23:23 18/10/19 STOP: 08:23   Thu Oct 18 12:16:39 2018, AT2, JLT, SN, 252Cf long measure, z=15cm beam upstream, no clovers  18/10/18 START: 20:20 18/10/18 STOP: 23:17   Thu Oct 18 08:21:18 2018, AT2, JLT, SN, 252Cf long measure, z=0cm, no clovers  18/10/18 START: 17:22 18/10/18 STOP: 20:09   Thu Oct 18 03:11:56 2018, AT & AT, bck meas  18/10/18 START: 10:54 18/10/1X STOP: 14:02   Thu Oct 18 00:31:55 2018, AT & AT, 252Cf long measure, z=0cm, threshold 5% lower  18/10/18 START: 08:31 18/10/18 STOP: 10:50   Wed Oct 17 14:11:18 2018, AT & AT, 252Cf long measure, z=0cm, threshold 5% lower  18/10/17 START: 22:04 18/10/17 STOP: 08:18   Wed Oct 17 09:20:20 2018, AT & AT, 252Cf long measure  18/10/17 START: 18:16 18/10/17 STOP: 22:00   Tue Oct 16 09:00:02 2018, ATD & JLT, Background measurement overnight  18/10/16 START: 16:56 18/10/17 STOP: 9:51   Tue Oct 16 08:57:56 2018, ATD & JLT, 252Cf source  252Cf source Run  START:? STOP: 16:56   Tue Oct 16 03:15:03 2018, ATD & JLT, Start of REP run preparation (RIBF148)  16-Oct-2018 - Start DACQ computer: OK!   Fri Dec 1 07:29:47 2017, Vi Ho Phong, [Hardware][Configuration] Return the PB-5 Pulse generator (Pulser 2) and the 428F Linear Fan in-out modules and replace with a new Linear Fan in-out module  7x The PB-5 Pulse generator labeled "Pulser 2" and the 428F Linear Fan in-out labeled "Clover G7" from BRIKEN NIM crate have to be returned to the RIBF electronics pool because the  borrowing time is expired.   Fri Nov 24 00:45:36 2017, AT, ur17b BRIKEN files  List of files in BRIKEN DAQ PC: Experiment DA1702 (including the test with YSO during first night)   Thu Nov 16 02:32:23 2017, BRIKEN collaboration, YSO thresholds  YSO Tests  Thresholds & calibrations   Tue Oct 31 06:57:53 2017, OH, TD, AIDA Oct17 Beam Test Analysis  PDF file attached with the preliminary analysis of the October 2017 AIDA in beam test.   Fri Oct 27 10:04:31 2017, SG, RY, LISE++ file for BRIKEN1  Here attached the lise file for BRIKEN1   Thu Oct 26 09:01:53 2017, BCR, Number of Counts vs Expected Efficiency for Proposals    Here is a doc with an estimate of the statistical uncertainty P1n and P2n as a function of the number of implant-beta correlations for future experiments.   Wed Oct 25 19:14:09 2017, NB, First pass efficiency for current experiment  I roughly (~10%) checked the efficiency for 4 of the peaks from  171025_1222_1355_152EuCloverCal.root. I checked the peaks at 122, 245, 344, and 1408. The indication is an efficiency of 6.9,  9,   9,8, and 2.6 % for these gamma rays repectively.   Wed Oct 25 18:12:43 2017, Sunflower collaboration, Gamma sources web page  http://www.nishina.riken.jp/collaboration/SUNFLOWER/misc/util/ribfsource.html   Wed Oct 25 17:49:09 2017, JT, AM, NB, DS, DM, AT, pulser in CLOVERS  G7 pulser weird behavior   Wed Oct 25 01:02:14 2017, RG, Status of the YSO array  The presently used detector has 48x48x5 mm3 YSO array with 1x1mm2 segments. They are separated with ESR.  We use H8500 pspmt and 2 mm quartz diffuser with rough edges. Coupling is done with sylgard.  Anger logic uses a conventional resistive network with 1kohm and we have 4 position signals and dynode.  The position signals (xa,xb,ya,yb) are split in Low gain branch connected directly to 5V range input in Struck and High gain branch, which   Tue Oct 24 13:14:47 2017, RY, Calibration data for clovers  for energy calibration with 152Eu source 171024_1858_152Eu_G7.root 171024_2112_152Eu_D4.root   Tue Oct 24 03:08:23 2017, RG, RY, MS, JA, RCF, SG, AT, light pulser YSO  light pulser measurement SN's pulse generator 20ns width   Mon Oct 23 09:43:00 2017, RG, RY, MS, SG, AT, 137Cs YSO  measurement of 137Cs with YSO  after matching the gains of the  HighGain channels   Sun Oct 22 11:32:59 2017, JA,ATD, JLT, New Gasific Configuration file      Sun Oct 22 11:14:35 2017, JA,ATD,JLT,RG,RY,SG,MS,PV,Liu,KR, 252Cf source Wasabi-BrikenYSO  252Cf source in the middle of Wasabi and YSO in front of Clover D4 Start: 19:15   Sun Oct 22 10:26:44 2017, JA,ATD,JLT,RG,RY,SG,MS,PV,Liu,KR, First Wasabi-YSO-BRIKEN correlation test  60Co source between YSO and Wasabi in front of D4 Clover Briken configuration file: 171022_1811_Conf_BrikenFullYSO.xlsx WRONG!!! Start: 18:25   Sun Oct 22 08:52:17 2017, KR,JA,ATD,JLT, Clover resolution  Resolution check using 40K 1460 keV line  in the background measurement overnight (File: 171022_0126_1101_bck.root)   Sun Oct 22 05:15:26 2017, RG,RY,MS,ATD,JA,JLT, Check of YSO 12x We start a systematic check of YSO in BRIKEN DACQ WE check and correct a configuration file for YSO alone   Sat Oct 21 17:30:23 2017, JA, ATD, JLT, Background measurement overnight  22/10/2017 Start: 01:26 Run: 037   Sat Oct 21 17:14:55 2017, JA, ATD, JLT, 252Cf efficiency calibration  Measurement of BRIKEN neutron counter efficiency 252Cf source in the (approximately) center Wasabi and D4 clover inserted. G7 on the floor.   Sat Oct 21 17:11:03 2017, JA, ATD, JLT, New Gasific configuration file  Configuration file saved on 22-Oct-2017 at 00:59 after increasing all the threshold in all 3He tubes to about 100keV. Also the threshold of Clover detectors was slightly increased.   Sat Oct 21 17:05:21 2017, JA,ATD, JLT, New DACQ hardware configuration  Configuration of BRIKEN DACQ hardware: Detector->VME->ADC->Channel   Sat Oct 21 07:26:13 2017, NB, RY, BD, MS, Corrected Calibration D4    K R G B m 0.001558636 0.0006599344 0.0015311753 0.0015807021 b -0.6545742444 0.4330534066 2.001278013 1.0994163913   Sat Oct 21 04:18:17 2017, NB, Draft of Instructions for HV  Setup: 2 MPOD + cards with 8 channels each one where the 10 BRIKEN PA are connected. 1 MPOD + card with 8 possible inputs   Fri Oct 20 08:27:05 2017, BC Rasco, Analysis Slides  Here are the ORNL/UTK BRIKEN analysis slides presented by BC Rasco on 2017/10/20.   Enjoy the fine reading.   Fri Oct 20 05:33:11 2017, KR, NB, SG, RY, JL, AT: , Calibration and Resolution of D4 (after Repair)   Green and Red channels were repaired by crimping and securing the grounding of the cables and fixing the cables securely to the table.  All problems during the repair process were visible on the scope. See example attatched.  Calibration is as:   Wed Oct 18 08:46:23 2017, NB, SG, AT, JL, Clover G7 resolution  G7 clover was on the stand Source: 152Eu File: 171018_1627_152Eu_G7.root   Mon Oct 16 05:52:14 2017, BRIKEN collaboration, START preparation  We start to check every thing for the coming run New directory: /data/1710Preparation/   Thu Jun 15 10:07:56 2017, BRIKEN collaboration, Gamma calibrations  Clover calibrations.  - Datafiles are located in the dac computer, path: /data/1706FinalCalibrations/GammaCalibration   Thu Jun 15 03:40:17 2017, BRIKEN collaboration, Z-scaning 252Cf Jun17  A scaning with 252Cf along the Z-axis of the neutron detector is carried out. The setup is similar to the scaning carried out in October 2016. Observations: - Clovers are put inside the detector without voltage.   Wed Jun 14 06:22:21 2017, Ariel, Liu, Go, Nishinmura, HV is off  To protect HPGe and 3He tubes from high intentsity primary beam, HV of these detector are off and the HPGe will be dismounted.   Tue Jun 13 08:02:35 2017, briken team, 133Ba calibration  After experiment 133Ba calibration Working directory: /data/1706FinalCalibrations Configuration file: 170604_Conf_BrikenFull_AfterCrisis.xlsx   Tue Jun 13 07:35:35 2017, briken team, 133Ba calibration  After experiment 133Ba calibration Working directory: /data/1706FinalCalibrations Configuration file: 170604_Conf_BrikenFull_AfterCrisis.xlsx   Tue Jun 13 06:50:12 2017, Briken Colaboration, 152Eu calibration  After experiment 152Eu calibration   Tue Jun 13 05:18:07 2017, PV, How to install ELOG for BRIKEN campaign 2017a   Get ELOG software including entries for BRIKEN campaign 2017a from mars computer: briken@mars:/data01/2017data/briken/ur17a/elogBRIKEN2017a.tar.gz   Mon Jun 12 22:28:02 2017, Oscar, The SUSHIRO app guide  It's here...it's rough...but it hopefully gets the job done   Mon Jun 12 02:45:44 2017, Iris Dillmann AT, Setup detectors. Id of Ancillary@BRIKEN  Attachment 1: Setup detectors  Attachment 2: example of configuration file (valid only for RIBF127). The Id of the ancillary detectors are:   Mon Jun 12 02:38:27 2017, JA AA AIM AT AT, VME crate & new configuration  Sun Jun 4 2017 11:16:45 VME crate #1 crashed New configuration file of BRIKEN   Mon May 29 07:06:56 2017, K. Matsui, Energy loss in Long Plastic Scintillator  After Al degrader with the optimized width of 13 mm, the energy loss in Long Plastic Scintillator is 546(2) MeV at F11. This value depends on    Mon May 29 05:40:49 2017, K. Matsui, energy loss at logn       Mon May 29 04:17:34 2017, YS, Clover Efficiency  Clover gamma detection efficiency calculation with 152Eu Date of the measurement: 2017-05-26 10:15 root file: 170526_1015_152Eu_noAIDA_z0cm_014.root   Sun May 28 11:41:24 2017, YS, CLOVER energy calibration  Clover calibration with 152Eu Used peaks [keV]: 121.7817, 244.6975, 344.2785, 444.000, 778.9045, 867.378, 964.100, 1112.074, 1408.011   Sat May 27 11:19:57 2017, AIM, AT, AIDA+BRIKEN background  Background measurement AIDA+BRIKEN AIDA is inside BRIKEN   Sat May 27 10:36:20 2017, JA,AT,JLT, BRIKEN DACQ  Manuals for BRIKEN DACQ:  GasificShort.pdf including "Run protocol" and Gasific70Manual.pdf (long)   Sat May 27 04:46:55 2017, AIM, sources info  Here is the sunflower webpage with information on the calibration sources: http://www.nishina.riken.jp/collaboration/SUNFLOWER/misc/util/ribfsource.html   Fri May 26 14:42:12 2017, JL, AT, Background  Background measurement (no AIDA)   Fri May 26 14:27:08 2017, AIM, AT, BRIKEN Configuration File  New configuration file of BRIKEN Changes of 26th-May-2017 Previous config file 24th-May-2017   Fri May 26 09:07:46 2017, J. Agramunt, Synchronization Monitoring  We started the synchronization monitoring programs to check that it is OK as can be seen in the figure below   Fri May 26 04:20:54 2017, JLT,AA,AT, CLOVER 60Co  60Co No AIDA, Efficiency calibration Start: 12:21   Fri May 26 03:52:23 2017, AT,AA,JLT, CLOVER, 137Cs  137Cs, No AIDA, Efficiency calibration Source ID: 393   Fri May 26 03:24:38 2017, GK,VP, AT, AA, CLOVER, 133Ba  133Ba source efficiency calibration, no AIDA Start: 11:23   Fri May 26 02:17:40 2017, AT, AIM, JLT,AA, PV, KM, 152Eu  Calibration with 152Eu source. START time:10:15   Thu May 25 14:31:46 2017, AT, JLT, AA, AIM, Background measurement 7x Background, No AIDA Start:22:31   Thu May 25 13:56:00 2017, AT, JLT, AA, 252Cf  252Cf source in Z=0cm position.  Start:21:57   Thu May 25 13:42:45 2017, AT, PC,KR,JLT,AA, 252Cf  252Cf source in Z=0cm position.  Start:21:41   Thu May 25 13:38:11 2017, AT, PC, KR, JLT, AA, Clover, detectors in new position  Both clover detectors were moved. They are in a symmetrical position. The end on the clover nose is of the order of 3-4 mm from the AIDA tunnel.   Thu May 25 13:24:02 2017, AT,PC,KR,JLT,AA, CLOVER, detector not in its rigth position  We have noticed that D4 is not in its right position. That explains the different number of counts in the detectors.  Probably of the order of 3 cm away from its nominal place.   Thu May 25 12:53:47 2017, AT, PC, JLT, KR, AA, Clover, 60Co  60Co source  Source ID: CD395   Thu May 25 12:49:55 2017, AT, JLT,PC,AA, Clover, 133Ba, LN2 filling  We started the measurement of the source when the N2 filling started. Just to  check if there are funny things related to the filling.   Thu May 25 10:15:02 2017, A.T, G. K, A.M, A. A, CLOVER, 133Ba no pulser  Source in position z=0 with the carton (cardboard) high-end, high-tech holder, but no AIDA (of course). No pulser. Remember that the pulser is providing peaks around    Thu May 25 09:51:37 2017, A.T, A.A, CLOVER, Ba133  Source details: Diameter: 25.05 mm   Wed May 24 13:22:46 2017, JLT,AT,KR,SG,RY,..., CLOVER 152Eu  We connect the pulser to both CLOVERs G7: It looks OK except for the G7-Green as before   Wed May 24 06:42:05 2017, JLT,AT,AM,RY,SG, START Preparation  We start to check every thing for the coming run New directory: /data/1705Preparation/   Sun Apr 2 16:18:57 2017, All, END OF PARASITIC RUN      Sun Apr 2 01:04:24 2017, JLT ID JA GK CG VP YS Liu, Background  Date: 2/04/2017  Start: 09:05 BRIKEN run: 76   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   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   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   Sat Apr 1 22:18:00 2017, Liu, YS, CG, GK, SN, JLT , 38Mg run 72  DUMMY   Sat Apr 1 21:37:42 2017, YS, Liu, CG, 37Na run 71  Date: 2/04/2017  Start:04:47 BRIKEN run: 71   Sat Apr 1 19:48:41 2017, YS,CG,LIU, 37Na,run 70  Date: 2/04/2017  Start:03:47 BRIKEN run: 70   Sat Apr 1 18:48:20 2017, YS, LIU, CG, 37Na run 69  Date: 2/04/2017  Start:02:47 BRIKEN run: 69   Sat Apr 1 17:45:01 2017, YS,CG,LIU, 37Na, run 68  Date: 2/04/2017  Start:01:44 BRIKEN run: 68   Sat Apr 1 16:17:59 2017, YS,CG, LIU, 37Na run 67  Date: 2/04/2017  Start:00:17 BRIKEN run: 67   Sat Apr 1 15:16:45 2017, JLT OH VP Liu YS, 37Na run 66  Date: 1/04/2017  Start:23:13 BRIKEN run: 66    Sat Apr 1 14:21:31 2017, PV OH Liu JLT, 37Na run 65  Date: 1/04/2017  Start:22:12 BRIKEN run: 65    Sat Apr 1 13:15:37 2017, JA ID OH PV, Na37 Ne36 Run 064  Date: 1/04/2017  Start:21:13 BRIKEN run: 63    Sat Apr 1 12:15:21 2017, PV, OH, JLT, ID, JA, 37Na run 63  Date: 1/04/2017  Start:20:15 BRIKEN run: 63    Sat Apr 1 11:13:42 2017, PV,OH,JLT, 37Na run 62  Date: 1/04/2017  Start:19:09 BRIKEN run: 62    Sat Apr 1 10:26:07 2017, VP,OH,JLT, 37Na run 61  Date: 1/04/2017  Start:18:25 BRIKEN run: 61    Sat Apr 1 10:15:44 2017, VP,OH,JLT, 37Na run 60  Date: 1/04/2017  Start:17:40  BRIKEN run: 60    Sat Apr 1 08:39:47 2017, ID OH JLT, 36Ne 37Na run 059  Date: 1/04/2017 Start:16:38 BRIKEN run: 59   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   Sat Apr 1 05:01:24 2017, ID DK GK JLT, 36Ne 37Na run 057  Date: 1/04/2017 Start:13:00 BRIKEN run: 57   Sat Apr 1 04:03:31 2017, ID JA DK GK, Na37 Ne36 run 056  Date: 1/04/2017 Start:12:00 BRIKEN run: 56   Sat Apr 1 02:07:49 2017, ID DK JA, Run 55  Date: 1/04/2017 Start:10:04 BRIKEN run: 55   Sat Apr 1 01:04:31 2017, ID DK JA, Na37 Ne36 Run 54  Date: 1/04/2017 Start: 09:03 BRIKEN run: 54   Sat Apr 1 00:04:10 2017, ID GK DK Liu, 37Na or 36Ne labels?  The BigRIPS settings are all called "36Ne setting" but the night shift labels these runs in the BRIKEN DAQ as "37Na". We are not sure why we label it with 37Na, we think this should be consistently named 36Ne like the BigRIPS settings. (For sure the strongest component in the beam might be 37Na. In the 39Na settings before it   Fri Mar 31 23:41:57 2017, ID, LIU, DK, GK, 37Na run 53  Date: 1/04/2017 Start: 07:41 BRIKEN run: 53   Fri Mar 31 22:45:21 2017, YS, LIU, DK, 37Na run 52  Date: 1/04/2017 Start: 06:45 BRIKEN run: 52   Fri Mar 31 22:22:40 2017, YS, LIU, DK, 37Na run 51  Date: 1/04/2017 Start: 06:23 BRIKEN run: 51   Fri Mar 31 21:45:25 2017, YS, LIU, OH, DK, 37Na run 50  Date: 1/04/2017 Start: 05:45 BRIKEN run: 50   Fri Mar 31 21:00:57 2017, YS, LIU, OH, 37Na run 49  Date: 1/04/2017 Start: 04:59 BRIKEN run: 49   Fri Mar 31 20:40:47 2017, YS, LIU, OH, 37Na run 48  Date: 1/04/2017 Start: 04:38 BRIKEN run: 48   Fri Mar 31 19:31:15 2017, YS, LIU, OH, CG, 37Na, run47  Date: 1/04/2017 Start: 03:30 BRIKEN run: 47   Fri Mar 31 18:28:54 2017, JLT, YS Liu, OH, CG, 37Na run 46  Date: 1/04/2017 Start: 02:46 BRIKEN run: 46   Fri Mar 31 18:00:41 2017, JLT,SN,JLiu,YS,CG, 37Na run 45  Date: 1/04/2017 Start: 01:57 BRIKEN run: 45   Fri Mar 31 16:56:16 2017, JLT, YS,Liu,PV,CG, New Configuration file  New configuration file:  170331_Conf_BrikenFull.xlsx   Fri Mar 31 15:30:24 2017, JLT, PV, Liu, SN, CG, 34Ne run 44  Date: 31/03/2017 Start: 23:27 BRIKEN run: 44   Fri Mar 31 14:40:56 2017, JLT, PV, Liu, CG, 34Ne run 43  Date: 31/03/2017 Start: 22:19 BRIKEN run: 43   Fri Mar 31 13:04:01 2017, JLT JA ID PV, 32Ne Run 42  Date: 31/03/2017 Start: 22:01 BRIKEN run: 42   Fri Mar 31 11:46:44 2017, ID PV CG, 40Mg Run 041  Date: 31/03/2017 Start: 19:43 BRIKEN run: 41   Fri Mar 31 10:35:22 2017, PV CG JA, Run 40  Date: 31/03/2017 Start:  BRIKEN run: 40   Fri Mar 31 09:23:45 2017, CG PV JA, Run 39  Date: 31/03/2017 Start: 17:22 BRIKEN run: 039   Fri Mar 31 08:23:32 2017, CG PV JA, Run 38  Date: 31/03/2017 Start: 16:21 BRIKEN run: 038   Fri Mar 31 07:17:03 2017, OH PV JA CG, Run 37  Date: 31/03/2017 Start: 15:24 BRIKEN run: 037   Fri Mar 31 05:27:44 2017, OH,SN,JA,PV, 40Mg run 36  Date: 31/03/2017 Start: 13:24 BRIKEN run: 036   Fri Mar 31 04:57:01 2017, ID,YS,JLT,OH, 40Mg run 35  Date: 31/03/2017 Start: 12:24 BRIKEN run: 035   Fri Mar 31 03:54:26 2017, ID JLT, Run 034: gamma spectra background lines  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.   Fri Mar 31 03:26:53 2017, ID OH SN, 40Mg Run 034  Date: 31/03/2017 Start: 11:23 BRIKEN run: 034   Fri Mar 31 02:26:19 2017, ID RCF, 40Mg Run 033  Date: 31/03/2017 Start: 10:23 BRIKEN run: 033   Fri Mar 31 01:50:15 2017, ID, RCF, 40Mg Run 032  Date: 31/03/2017 Start: 10:01 BRIKEN run: 032   Fri Mar 31 01:01:58 2017, ID RCF OH, Run 031  Date: 31/03/2017 Start: 08:58 BRIKEN run: 31   Fri Mar 31 00:01:55 2017, ID JA DK GK Liu, Run 030  Date: 31/03/2017 Start: 07:58 BRIKEN run: 30   Thu Mar 30 22:19:22 2017, Liu DK KG JA ID, Run 28-29  Date: 31/03/2017 Start: 06:30 BRIKEN run: 28   Thu Mar 30 21:01:54 2017, JA DK KG Liu, Run 27  Date: 31/03/2017 Start: 5:04 BRIKEN run: 27   Thu Mar 30 20:13:11 2017, JA, GK, DK, 40Mg run25  Date: 31/03/2017 Start: 04:13 BRIKEN run: 25   Thu Mar 30 19:16:46 2017, GK,DK,JLiu,JA,JLT, 40 Mg run 24  Date: 31/03/2017 Start: 03:14 BRIKEN run: 24   Thu Mar 30 18:14:59 2017, JLT,DK,GK, Liu, 40Mg run23  Date: 31/03/2017 Start: 02:14 BRIKEN run: 23   Thu Mar 30 17:17:21 2017, JLT,GK,DK,JLiu, 40Mg run 22  Date: 31/03/2017 Start: 01:14 BRIKEN run: 22   Thu Mar 30 16:15:24 2017, SN, JLT, GK, DK, JLiu, 40Mg run 21  Date: 31/03/2017 Start: 00:12 BRIKEN run: 21   Thu Mar 30 13:35:30 2017, JLT,TD, JLiu,SN, GK, 40Mg run 20  Date: 30/03/2017 Start: 21:33 BRIKEN run: 20   Thu Mar 30 12:27:44 2017, JLT,TD,JLiu,SN, 40Mg run 19  Date: 30/03/2017 Start: 20:26 BRIKEN run: 19   Thu Mar 30 11:35:52 2017, JLT,TD,PV,JLiu, 40Mg run 18  Date: 30/03/2017 Start: 19:33 BRIKEN run: 18   Thu Mar 30 10:26:06 2017, JLT,TD,PV, 40Mg run 17  Date: 30/03/2017 Start: 18:24 BRIKEN run: 17   Thu Mar 30 09:24:45 2017, JLT,RC,TD,PV,SN, 40Mg run 16  Date: 30/03/2017 Start: 17:22 BRIKEN run: 16   Thu Mar 30 07:41:58 2017, RCF PV SN CG JA, Run 15  Date: 30/03/2017 Start: 16:05 BRIKEN run: 15   Thu Mar 30 07:31:09 2017, SN PV CG RCF JA, Run 14  Date: 30/03/2017 Start: 15:30 BRIKEN run: 013   Thu Mar 30 06:30:06 2017, JA CG PV SN, Run 13  Date: 30/03/2017 Start: 14:25 BRIKEN run: 013   Thu Mar 30 05:56:28 2017, JLT,JA,CG,PV, 40Mg Run 12  Date: 30/03/2017 Start: 13:54 BRIKEN run: 012   Thu Mar 30 04:49:52 2017, JLT,TD, 40Mg Run 11  Date: 30/03/2017 Start: 12:47 BRIKEN run: 011   Thu Mar 30 03:55:42 2017, J. Agramunt, 40Mg Run 10  Date: 30/03/2017 Start: 11:52   Thu Mar 30 01:46:30 2017, J.Agramunt, 40Mg Run 009   Date: 30/03/2017 Start: 09:47   Thu Mar 30 00:47:04 2017, J. Agramunt, 40Mg Run 008   Date: 30/03/2017 Start: 08:41   Wed Mar 29 22:53:58 2017, J. Agramunt, 40Mg Run007   Date: 30/03/2017   Wed Mar 29 21:34:20 2017, RCF, 40Mg Run 006   Date: 30/03/2017   Wed Mar 29 20:27:53 2017, RCF, 40Mg Run005   Date: 30/03/2017   Wed Mar 29 19:31:21 2017, RCF, 40Mg Run 004   Date: 30/03/2017   Wed Mar 29 18:42:25 2017, RCF, 40Mg Run 003   Date: 30/03/2017   Wed Mar 29 18:16:58 2017, RCF, 40Mg Run 002  Date: 30/03/2017   Wed Mar 29 17:15:21 2017, JLT, New Config file  New configuration file: 170330_Conf_BrikenFull.xlsx   Wed Mar 29 15:16:17 2017, Many, 40Mg Run 001  Date: 29/03/2017 Start: 23:13   Wed Mar 29 14:14:58 2017, Many, 40Mg RUN 000  Date: 29/03/2017 Start: 22:13   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  Start of parasitic Ca beam (main experiment "New isotope search", Ahn et al.)   Wed Mar 29 11:02:40 2017, PV, Liu, JA, JLT, F11 plastic  New calibration of F11 plastic We decided to have both a low gain and a high gain    Wed Mar 29 07:34:16 2017, J. Agramunt, BrikenTools repository installed at d05  The last version of Briken tools repository has ben installed at d05, this repository includes the Merger and the BrikenOffline codes, as well as a CommonTools folder to share scripts and code. For update versions, just type in the desired directory "svn update".   Wed Mar 29 03:02:02 2017, J. Agramunt, Synchronization test procedure (update)   To Launch the processes: Open 4 terminals:   Tue Mar 28 17:02:19 2017, DK, Applying Biases  Today, Gabor and I discussed with Nathan from ORNL about the biasing system used for Ge, 3He, Plastic, and others.  Phong is also a bit familiar with the system (edit also  Shintaro    Tue Mar 28 09:10:09 2017, Many, 152Eu  152Eu source inside BRIKEN for CLOVER calibration. Also calibration of Si-dE with 60Co source and AIDA_PL calibration  with 60Co source.   Tue Mar 28 06:56:15 2017, PV, Liu, JA, JLT, F11 Plastic  Calibration of new F11 plastic (see photo)   Mon Mar 27 11:53:15 2017, PV,Liu, Turn on dE detector  We applied a bias voltage of 100 V to the dE detector Current read = 0.660 uA compare with https://elog.ph.ed.ac.uk/BRIKEN/190.  it is slighly lower.   Mon Mar 27 09:32:55 2017, JLT JA CG OH DK TD RC VP GK LJ SN, 252Cf  252Cf at the center for BRIKEN calibration   Mon Mar 27 03:50:13 2017, JLT JA CG OH DK TD RC VP SN, Background  Background measurement while they play with the beam. Start: 11:40   Sat Mar 25 13:42:23 2017, JL Tain, J Agramunt, V. Phong, C. Griffin, O. Hall, S. Nishimura, R. Caballero, Background  BRIKEN system powered and DACQ started after movement. All looks fine.   Sat Mar 25 13:33:12 2017, JL Tain, J Agramunt, V. Phong, C. Griffin, O. Hall, S. Nishimura, R. Caballero, BRIKEN+AIDA relocated  We moved AIDA+BRIKEN by 107cm upstream. See attached photos.   Fri Mar 24 03:28:39 2017, JL Tain, J Agramunt, V. Phong, C. Griffin, O. Hall, S. Nishimura, Background  Background measurement overnight Start: 19:45   Thu Mar 23 10:03:51 2017, JL Tain, J Agramunt, V. Phong, C. Griffin, O. Hall, S. Nishimura, 252Cf  252Cf source at the center for calibration 23/03/2017   Thu Mar 23 09:30:58 2017, JL Tain, J Agramunt, V. Phong, C. Griffin, O. Hall, S. Nishimura, Power-up and 1st spectrum  Crates powered up. DACQ started. New directory: /data/1703Preparation/   Thu Mar 23 09:04:38 2017, JL Tain, J Agramunt, V. Phong, C. Griffin, O. Hall, S. Nishimura, Remove EURICA rails  We remove partially the floor rails of EURICA  to proof that it is possible to move BRIKEN + AIDA.   Thu Mar 23 09:01:33 2017, JL Tain, J Agramunt, V. Phong, C. Griffin, O. Hall, S. Nishimura, ELOG Start Preparation  We started the preparation of 2017 campaign   Fri Dec 9 05:25:26 2016, PV, Photo and schematic drawing of the Pb shielding in front of BRIKEN during Fallon experiment  This Pb shielding structure is right behind the variable degrader   Thu Dec 8 04:17:49 2016, PV, Installing BRIKEN ELOG 2016 in RIBF local network to a personal computer  All the RIBF123 elog website (including Takechi and Fallon experiment) can be downloaded and installed from the following link: https://drive.google.com/file/d/0B5rBCXKaAWNARVViSTBNSE80RzQ/view?usp=sharing To run and view the elog website in your local computer (tested with Centos 7, it may work with Ubuntu or any other linux distro)   Tue Nov 29 00:30:42 2016, PV,SN, Sillicon dE bias voltage increased  We increase the bias voltage of the dE detector from 20 V to 100 V Leakage current: Before: ~0.590 uA   Mon Nov 28 16:18:07 2016, AE, DAQ synchronization   Please see: https://elog.ph.ed.ac.uk/AIDA/493   Mon Nov 28 10:48:21 2016, JLT, Online analysis  Comparison of current spectra with spectra from Takechi's run (See attachment)   Mon Nov 28 05:59:28 2016, briken , run  =======    START    ======= Date 2016/11/28 Start time : 11:12 BRIKEN run : 056 Daq Conf. File : 161128Conf_BrikenFull.xlsx DLT File name : 161128_1112 AIDA run : R28-0 AIDA start : 11:08 BigRIPS run : 1049 BigRIPS start : 09:15   --------------------------- Shifters:  AT GK KD =======    Setup    ======= Central fragment:  41Al @F8 --- Degraders ---  Fixed: 3mm Pb between Musics chambers  Included lead shieldings around the beam.   Mon Nov 28 01:22:50 2016, BRIKEN collaboration, Elog RIBF123 & BigRIPS 6x Full RIB123 Elog entries for Takechi && Fallon parasitic experiments Update:03Dec16 Instructions:   Sun Nov 27 23:14:49 2016, BRIKEN coll, run 036  =======    START    ======= Date 2016/11/27 Start time : 19:28   Sun Nov 27 11:23:54 2016, PV, GK, AE, TD , 40Mg. Run 35   =======    START    ======= Date 2016/11/27 Start time : 18:59   Sun Nov 27 11:15:42 2016, PV, GK, AE, TD , 40Mg. Run 34  =======    START    ======= Date 2016/11/27 Start time : 17:29   Sun Nov 27 11:07:02 2016, PV, GK, AE, TD, 40Mg. Run 33 - junk  =======    START    ======= Date 2016/11/27 Start time : 17:17   Sun Nov 27 10:47:20 2016, PV,TD,GK, 40Mg. Run 32  =======    START    ======= Date 2016/11/27 Start time : 16:20   Sun Nov 27 07:10:29 2016, BRIKEN colaboration, Run 31  =======    START    ======= Date 2016/11/27 Start time : 13:53   Sun Nov 27 04:38:15 2016, BRIKEN collaboration, Run 030  =======    START    ======= Date 2016/11/27 Start time : 10:41   Sun Nov 27 04:36:16 2016, BRIKEN collaboration, Run 020-023  =======    START    ======= Date 2016/11/26 Start time : 20:05   Sat Nov 26 20:50:13 2016, GK, AT&AT, run 16-19  =======    START    ======= Date 2016/11/26 Start time : 17:21   Sat Nov 26 20:48:16 2016, BRIKEN collaboration, run  =====   Start of measurements 41Al  ======   Sat Nov 26 16:54:17 2016, AT & AT, Clovers  Calibration of clovers   Sat Nov 26 16:21:08 2016, Briken collaboration, 41Al run 2-15  13:08 Beam is still OFF. Background acquisition is started. Degrader: 3 mm Pb   ONLY!   Sat Nov 26 09:31:05 2016, Gabor Kiss, Ariel Tarifeno, Alvaro Tolosa, Output signals from G7Red  Preamplifier of crystal G7Red was replaced.  Output signals from G7Red are weird.   Sat Nov 26 06:37:37 2016, AT, 41Al run 1  11:07  New acquisition is started for tungsten degraders  1mm W + 1mm Al 0.5mm W + 1mm Al    Sat Nov 26 06:30:30 2016, AT, Setup  Setup for parasitic experiments Energy 41Al @ F11 is around 145MeV/u   Sat Nov 26 00:15:12 2016, AT, 41Al run0  08:15    BigRips tunning for centering 41Al. Adqusition started. Degrader: 5mm Pb located between MUSIC chambers   Sat Nov 26 00:04:15 2016, AT, Elog  RIKEN Elog during Fallon Parasitic experiments Fallon Group:    Fri Nov 25 23:18:04 2016, BRIKEN collaboration, Fallon Parasitic experiments  =====   START OF PARASITIC EXPERIMENTS  ======   Fri Nov 25 21:50:42 2016, AT, New Conf File  161125Conf_BrikenFull.xlsx   Fri Nov 25 21:49:36 2016, AT, Background Beam OFF  21:27  Beam off. Background is started. 22:10  Acquisition is stopped. Files:   Fri Nov 25 21:48:49 2016, AT, DACQ  19:00  Test calibration    Fri Nov 25 21:47:05 2016, AT, Background Beam OFF  16:17  Background beam OFF 16:27 Beam On. Acquisition stopped just after beam ON. File:   Fri Nov 25 03:49:44 2016, AT, Background Beam ON  16/11/25 12h28min: Background measurement beam ON 19B   Fri Nov 25 03:41:40 2016, AT, Run setups  Run setups during preparation of Fallon Parasitic experiments (Kanungo experiment beam time) can be found on  http://ribfdaq/~gamma16/expdbrunsum.php   Fri Nov 25 03:37:23 2016, AT, Background Beam OFF/ON  16/11/24 21h06min: Background measurement Beam OFF + Beam ON tunning and 22C 21:41 : Until now Beam OFF, BigRips team tunning the machine. An online is saved    Fri Nov 25 03:15:46 2016, AT, Background Beam ON  16/11/24 19h38min:   Background measurement during tunning of BigRips from 27-29F to 22C is started.   Thu Nov 24 14:57:55 2016, AT, Background Beam ON  Starting from today 12:22, the background generated by the different setups on BigRips is monitorized. - 30 min aprox Beam off   Thu Nov 24 14:36:27 2016, AT, 252Cf  Check of calibrations and rates for neutron detectors with Conf File 161107Conf_BrikenFull.xlsx Measurement 161122_2208_003.root has been used to check the calibrations and counting rates in the BRIKEN   Thu Nov 24 02:30:56 2016, CG, RIBF123R1 Local ELogs 9x PDFs of the local ELog for the RIBF123R1 experiment Nov 2016   Tue Nov 22 10:22:07 2016, PV, Liu, No current observed when turning on the HV for the D4 Clover  19:00 We've turned on the High Voltage for the D4 Clover up to ~ 1.5 kV.  There is no current (0.0 uA) observed in all the channels (crystals) of this clover while the High Voltage is   Tue Nov 22 10:17:57 2016, ATS, PV, LIU, 252Cf  Measurement with 252Cf at Z=22.5cm from the moderator border, opposite side from AIDA. Clovers and Veto detectors are turned off. Beam is off.   Tue Nov 22 09:26:04 2016, A. Tarifeno-Saldivia, Noise check  Run for checking the noise just after turn on the crates, without high voltages on the PREAMPS. Attached calibrated histogram for the full BRIKEN detector.    Tue Nov 22 08:28:36 2016, A. Tarifeno-Saldivia et al, New directory and Config File  A new directory in the IFICdaq computer has been created for the parasitic measurements during the Fallon Beam Time. The path of the folder is:   Sun Nov 20 13:02:06 2016, Jorge, Alavaro, Jose, DACQ  Gasific-7.0 Short Manual (Preliminary)   Sun Nov 20 12:28:27 2016, Jorge, Alvaro, Jose, DACQ  Updated run protocol   Fri Nov 11 08:07:18 2016, BCR SG NTB, BRIKEN Hit Visualization  These are the files used to create and visualize the hit patterns of the BRIKEN detector. There are three files needed plus one input data file. The three files are "HybridBRIKENPhysicalHistogram.hpp", "HybridBRIKENPhysicalHistogram.cpp", and "HybryidBRIKEN_Tube_Info_1.txt". These files are attached to this eLog entry.   Thu Nov 10 05:05:54 2016, KM, How to convert ridf-file to root-file  1. Login to briken@ribfana03.riken.jp 2. Check if the ridf-file you want to convert is in the directory; /home/briken16/rawdata/bigrips/ 3. Login to anaroot; type "anarootlogin"   Wed Nov 9 02:02:22 2016, Iris, Boron rubber from India  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   Tue Nov 8 06:13:11 2016, Tain et al, New plastic detector in F11  There is a new plastic scintillator after the MUSIC chambers       Tue Nov 8 06:39:25 2016, Tain. Iris, Drawing of present setup  Attached is the present setup including all walls, auxiliary detectors, degraders etc. and the Takechi setup.   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/    Tue Nov 8 17:00:27 2016, NTB, CG, AT, Si Delta E  At least during the timeframe in between ~ 21:30 (11/08) - 23:30 (11/09) (161108_2323_717273Ni.root) we see that the silicon dE have a very low counting rate. ~1Hz when the first AIDA detector sees ~600 Hz and a cumulative ~2kHz. The energy range in the dE stops at ~10MeV. Edit: It appears the Si dE were removed. Some signals are still in the spectra.   Tue Nov 8 15:10:24 2016, Many, 717273Ni Run  F7 OUT F11 C-6mm Start: 00:09   Tue Nov 8 14:28:54 2016, Many, 717273Ni run  F7 CH2 F11 C-6mm Total degrader thickness 6mm   Tue Nov 8 13:49:58 2016, Many, 71,72,73Ni  F7 CH2 F11 Empty We remove the 8mm Al plate from inside BRIKEN infront of AIDA   Tue Nov 8 12:51:08 2016, Many, 717273Ni   After removing the lead wall. Start: 21:45   Tue Nov 8 12:30:33 2016, Tain, Ale (who are not on shift), 71,72,73Ni run  71,72,73Ni  run We started at approximately 21:00, only online, not writing on tape.    Tue Nov 8 11:51:28 2016, Ale, spikes on some spectra  Some spectra show spikes or do not look normal. This should be checked. Look at BRIKEN, Ring4, Ring5, Ring6, Ring7, D4, G7, Clovers,    Tue Nov 8 08:49:51 2016, Tain et al, Move ELOG  We will start to use the internal RIKEN ELOG It is not clear that we can keep the present ELOG also updated   Tue Nov 8 08:31:52 2016, Tain et al, 424344Ca run  Sequence of settings: 1) No target at F7 and Empty target at F11 (up to t=1E6ms) 2) No target at F7 and C-6mm target at F11 (up to t=5.1E6ms)   Tue Nov 8 02:49:19 2016, PV, Liu, Specification of the dE silicon detector  The specification and picture of the dE silicon detector is shown in the attached photos. The detector  has an effective area of 134 x 123 mm and  320 micrometer  thick There are 26 vertical strips. They are combined into 2 readout channels (top and bottom which respect to the orientation of the detector in BRIKEN)   Mon Nov 7 14:17:23 2016, BRIKEN collaboration, Picture of shift schedule      Mon Nov 7 13:44:26 2016, Alvaro, Ale, Jorge, Jose, Running Gasific and run protocol  Preliminary   Mon Nov 7 13:15:07 2016, Alvaro, Ale, Jorge, Jose, Background  Background measurement overnight. Start: 23:27 (07/11/2016)   Mon Nov 7 13:11:42 2016, Alvaro, Ale, Jose, Jorge, New directory and Config file  For second part of Takechi's run: Directory: /data/1611Commissioning/161107Parasitic   Mon Nov 7 09:05:09 2016, Iris, Draft for Run sheet  Attached is the draft for the paper run sheet (version 2). If something is missing, please let me know.   Mon Nov 7 09:04:10 2016, Phong,Liu,Ale,Jose, New AIDA plastic calibration  To have a range of about 200 MeV Ortec671 Gain from x20 to x5 (fine gain : x0.5)   Mon Nov 7 06:55:01 2016, NTB, SG, HPGe Fill line to D4 replaced  HPGe fill line to D4 replaced only small leak (overflow) once Ge is full. Solenoid was also wrapped to no effect. AIDA DAQ still stops writing. Boron sheet and extra polyethylene were placed back on top.   Mon Nov 7 05:36:20 2016, Ale, new calibration for F11  new calibration for F11 Using a value of 70 MeV energy loss and the file 161107_0833_Overnight.root   Mon Nov 7 04:49:57 2016, Tain, Ale, AIDA plastic (veto) and Si de calibration  AIDA plastic (veto) and Si de calibration For the calibration the Compton edge of the spectrum seen in the detectors was used.   Mon Nov 7 04:37:33 2016, Phong,Liu,..., Si de and AIDA plastic calibration  60Co source placed close to the detectors: ROOT files:    Mon Nov 7 02:39:55 2016, Ale, Photo of the white board with the details on the cards and preamps at B1F  Photo of the white board with the details on the cards and preamps at B1F   Sun Nov 6 23:35:42 2016, Tain et al., Overnight measurement: Ca isotopes  First 50,49,48Ca beam and then 47,46,45Ca beam C-6mm IN and OUT   Sun Nov 6 07:16:59 2016, Tain et al., 58Ni on F7 CH2 F11 empty/C6mm  CH2 target at F7 in Start with Empty at F11 Change to C-6mm at F11 later   Sun Nov 6 06:39:23 2016, Tain et al., 58Ni on F11 C-6mm  58Ni in F11 C-6mm (later empty) F7 CH2 target out (F5 CH2 target in) Thresholds in V_PL_* lowered from 20MeV to 1MeV   Sun Nov 6 06:27:49 2016, Tain et al., 58Ni on F11 C-6mm in  New calibration in V_PL_T and V_PL_R (Energyx1/2) Start: 15:15   Sun Nov 6 03:12:55 2016, Alvaro,Jorge, Overnight measurement  Measurement during beam production and measurement with F7 CH2 out,  F11 C-tar in/out, F7 CH2 in C-target out/in   Sat Nov 5 17:07:27 2016, Tain, Alvaro, Jorge, 62Ni in F7  62Ni beam in F7 ON CH2 target Strat with C target ladder in F11 in empty position.   Sat Nov 5 16:27:13 2016, Tain,Ale,Jorge,Alvaro, 62Ni beam in F11 empty target  Empty position of the target ladder at F11 (hole is smaller than beam size)   Sat Nov 5 15:07:11 2016, Tain, Ale, 62Ni beam on F11 C-6mm  62Ni on 6 mm C target between MUSICs The background before was 0.36 neutrons/s   Sat Nov 5 03:36:34 2016, Tain et al, Ancillary detectors  Some info on ancillary detector signals Plastic veto detectors (Top and Botomm):   Sat Nov 5 03:18:13 2016, SG BCR RCF NTB, Gamma peaks in the overnight run, related to neutron inelastic scattering  We looked at the overnight background run (161105_0935_BackgroundOvernight.root), There are gamma-peaks that could be related to neutron inerastic scattering. We identified 565, 596, 608 and 69 keV. They might be related to the effect of neutrons. If this is the correct assignment, this would mean at least some of the neutrons are not thermal when they interact with the germanium.    Sat Nov 5 01:26:46 2016, Jose,Iris,Alvaro, Alejandro, Krzysztof, Background measurement 7x Measurement overnight Start: around 1:00   Sat Nov 5 01:25:24 2016, Tain et al, End of Beam Line Setup 9x Some photos of the elements in the last part of the beam line during Takechi run.   Fri Nov 4 13:16:42 2016, JLTain,ATolosa,JAgramunt, Neutron Background  Beam tuning in BigRIPS At 19:00 access to Exp. Area was closed and the tuning   Thu Nov 3 05:27:48 2016, Alvaro, Tain, Gabor, Ale, 152Eu   Energy calibration for clovers, 152Eu       Fri Nov 4 03:37:27 2016, Roger Caballero, Energy calibration for Ge clovers  Energy Calibration: See attached pdf Detector Slope Offset   Thu Nov 3 23:28:01 2016, A. Tolosa, BRIKEN Bkg + 152Eu  Measurement over night with a 152Eu source inside Start: 22:48 (03/11/2016)   Thu Nov 3 15:09:52 2016, A. Tarifeno-Saldivia, C. Domingo-Pardo, J.L. Tain, BRIKEN neutron efficiency  Geant4 BRIKEN Neutron efficiency calculations as a function of neutron energy and for some spectra: Ga84-vandle, Br88-endf71, Rb94-endf71, Rb95-endf71, I137-endf71, Cf252-MCNPX      Thu Nov 3 14:02:49 2016, Nepal, J Ha, PV, Liu J, The degrader system has been set  We used the laser to align the degrader (see attached photos) According to the LISE calculation, equivalent effective thickness for 6 mm of Carbon target is 4.5 mm thick Aluminum. Therefore, we've set the degrader system as follow:   Thu Nov 3 05:46:48 2016, Iris, Ale, Background measurement  Background measurement for threshold determination   Thu Nov 3 04:46:24 2016, Alvaro Tolosa, 252Cf  Check of BRIKEN calibration and thresholds Source more or less at the center   Thu Nov 3 04:40:02 2016, All, START  Start of commissioning preparation   Tue Nov 1 09:27:02 2016, Alvaro Tolosa, CLOVER  Efficiency calibration File "cloversEff.ods" and "cloversEff.xls" contains the experimental efficiency from different measurements       Tue Nov 1 13:00:55 2016, Roger Caballero, Eff callibration parameters for G7-Clover  Efficiency calibration for the G7 clover (data acquired in July). The attached plots show the parameters for the Jackel function (E[i]=Energy) using the points of a 152Eu source.       Wed Nov 2 01:19:46 2016, Roger Caballero, Eff callibration parameters for D4-Clover  Efficiency calibration for the D4 clover (data acquired in October). The attached plots show the parameters for the Jackel function (E[i]=Energy) using the points of 152Eu, 60Co and 137Cs sources.       Wed Nov 2 02:26:22 2016, Roger Caballero, Efficiency callibration calculator (Excel file)  Attached the updated excel file. In the first sheet there is the calculator to calculate the efficiency from an given energy. The Jackel function used is:   Mon Oct 31 23:56:37 2016, J. Agramunt, First AIDA BRIKEN correlation plot  From the 252Cf data.   Tue Oct 18 09:41:43 2016, Alvaro Tolosa, 2016 - July, Logbook  Paper logbook for July-2016 For correct visualization,  please download it.   Tue Oct 18 09:36:07 2016, Alvaro Tolosa, 2016-Oct, Logbook  Paper logbook for October-2016 For correct visualization,  please download it.   Mon Oct 17 05:21:46 2016, Phong, Liu J J, dE detector position and output signal from preamplifier  dE detector is mounted onto the back side of the shielding (attached photo: dE_position.JPG) The detector consists of 26 strips. In this setup, the detector is devided into 2 parts corresponding to 2 readout channels. Each part consists of 13 strips   Sun Oct 16 13:30:43 2016, All, END  ... and sashimi (see photo) The detectors (BRIKEN tubes, CLOVER, VETO detectors, AIDA)    Sun Oct 16 12:58:34 2016, All, BRIKEN  Installation of BRIKEN PE shielding for beam related neutrons   Fri Oct 14 14:06:38 2016, All, First measurement of BRIKEN and AIDA  Friday, October 14, 2016 21:50 AIDA and BRIKEN-CLOVER run with a common clock.   Fri Oct 14 13:32:52 2016, NT BREWER, S Go, JM Allmond, Ge preamp power loss and solution.   As previously recorded (81), on Thur Oct 13th, A NIM crate failure caused preamp power loss to the HPGe's. While D4 recovered with nominally the same resolution as before. G7 would not recieve power to the preamps without an alarm from the NIM crate. It was determined that there was a short along the lines of +12V and Ground , -12V and Ground, and between +-12V.   Fri Oct 14 04:42:40 2016, JL Tain et al, Electronics  Change of main power line for MPOD and CLOVER preamp   Fri Oct 14 04:12:50 2016, JL Tain et al, CONF  New configuration file:  161014Conf_BrikenFull.xlsx   Thu Oct 13 23:42:27 2016, JL Tain et al, Background  Background measurement overnight Start: 01:17   Thu Oct 13 23:41:25 2016, JL Tain et al, 252Cf  New BRIKEN energy calibration   Thu Oct 13 23:39:58 2016, JL Tain et al, VETO Det  Energy calibration of plastic and NaI detectors   Thu Oct 13 23:38:26 2016, JL Tain et al, CLOVER  Energy and efficiency calibration We make calibrations for the remaining D4 CLOVER detector   Thu Oct 13 12:58:31 2016, JL Tain et al, INCIDENT  NIM Crate Failure. Lost of CLOVER G7 One of the 2 NIM crates, the one containing the power for CLOVER   Thu Oct 13 04:36:58 2016, JL Tain et al, CLOVER  CLOVER energy calibration Short run with 137Cs and 60Co sources at BRIKEN detector center   Wed Oct 12 11:30:53 2016, Ariel Tarifeno, Alvaro Toloza, JL Tain, J. Agramunt, et al, BRIKEN Z scan  Scanning of the BRIKEN detector with the 252Cf source  along the longitudinal axis (Z axis)   Wed Oct 12 05:06:57 2016, JL Tain et al, Noise  Gamma source close to ORNL2 tube In order to investigate the origin of the background   Wed Oct 12 03:47:14 2016, JL Tain et al, Background  Background measurement over night with CLOVER and VETO detectors ADC #7 added to crate 1 for veto detectors: V1A7   Tue Oct 11 17:11:28 2016, A. Tarifeno-Saldivia et al..., ROOT macro   ROOT macro for calculation of neutron rates in the BRIKEN detector Here a ROOT macro to calculate neutron rates from onlines root files generated DAQ configuration    Tue Oct 11 15:58:01 2016, JL Tain et al, VETO Det  Check of Plastic and NaI veto detectors and DACQ settings   Tue Oct 11 15:47:45 2016, N Brewer, S Go et al, CLOVER  Both COVER detectors are installed in place. See photos.   Sun Oct 9 18:19:01 2016, JL Tain et al, Noise  Optimization of ADC thresholds In order to try to reduce the grass-like background   Sun Oct 9 15:49:41 2016, JL Tain et al, Power shutdown  Due to maintenance operations of the Wako electrical company there is a risk of power shutdowns on Saturday, Sunday and Monday from about 8 am to 8 pm.   Sun Oct 9 04:20:47 2016, JL Tain et al, Noise  We check for the appearance of spurious signals in the preamplifiers. We set all HV to zero and run a measurement for several hours.   Sat Oct 8 01:18:51 2016, JL Tain et al, DACQ  We increased the pretrigger delay for ADC5 from 350 to 400   Fri Oct 7 10:42:52 2016, JL Tain et al, Noise  We investigate the effect on the noise in ORNL tubes of using a differential PA. We connect the tubes in current PA10 (126-140) to one of the new diff PA   Fri Oct 7 08:35:15 2016, JL Tain et al, Noise  Low amplitude noise component. The figure shows the composition of the low amplitude noise   Fri Oct 7 08:09:47 2016, JLTain et al, Background  Background measurement overnight Start: Oct-6 2242 Stop: Oct-7 10:45   Thu Oct 6 14:50:30 2016, JL Tain, A Tolosa, A Tarifeno,..., 252Cf  First measurement with 252Cf source to check the calibration. AIDA was in place so the source was at the right height but displaced about 10cm from the center.   Thu Oct 6 14:43:47 2016, JL Tain, A Tarifeno, A Tolosa, J Agramunt, N Brewer, S Go, ..., Electronics  We mount back all preamplifiers Initially we used all the PA coming from US, the repaired and the new ones. There was an issue with the new ones (strong noise and cross talk)   Thu Oct 6 02:03:32 2016, JL Tain, START 6x We started the assembly of BRIKEN and AIDA detectors in their final position on Tuesday October 4:   Thu Aug 18 23:32:59 2016, NT Brewer, New preamps arrived at Oak Ridge and tested working.  Collaborators, Attached is a phone photo of example signals from the new preamps with 3 3He tubes connected to a scope. Scope channels 1,2,3 (color y,c,m respectively) are preamp channels 1,2,3 while 4 (green) is open. Trigger is on channel 3, at 500mV/div and other channels are at 500,200,and 20 mV/Div for channels 2,1,4   Thu Aug 18 22:39:35 2016, NT Brewer, New preamps arrived at Oak Ridge and tested working.  Collaborators, Attached is a phone photo of example signals from the new preamps with 3 3He tubes connected to a scope. Scope channels 1,2,3 (color y,c,m respectively) are preamp channels 1,2,3 while 4 (green) is open. Trigger is on channel 3, at 500mV/div and other channels are at 500,200,and 20 mV/Div for channels 2,1,4   Fri Jul 29 09:52:28 2016, Keishi Matsui, accuracy of Cf-252's intensity in RIKEN   According to the reply from Japan Radioisotope Association, the accuracy of the Cf-252's intensity is +0%/-15%. ( "+0%" is important, because 3.7 MBq is a standard limit for radio-active sources  in Japan.)   Fri Jul 22 12:50:29 2016, J.L. Tain, END  20/JUL/2016 20:00  End of the test measurements   Wed Jul 20 17:21:59 2016, J. Agramunt, A. Tolosa, DACQ  DACQ configuration parameters The last configuration file used was: 160718Conf_BrikenFull_cal5.xlsx   Wed Jul 20 17:18:59 2016, J.L. Tain, J. Agramunt, A. Tarifeņo, A. Tolosa, K. Gabor, S. Go, K. Matsui..., Electronics  Measurement with preamplifiers after drying. Amplifiers are brought back after ~12h and connected.   Wed Jul 20 17:05:59 2016, J.L. Tain, J. Agramunt, A. Tarifeņo, A. Tolosa, ..., Background  Background measurement with remaining tubes (95) overnight Listmode: 160719_2343_Bkg_*.dlt, Run: 031-044   Wed Jul 20 16:55:48 2016, K.Gabor, K. Matsui, A. Tarifeņo, Electronic  Drying of preamplifiers PA8, PA9 and PA10 are removed and brought to a dryer box   Wed Jul 20 16:50:12 2016, J.L. Tain, J. Agramunt, A. Tarifeņo, A. Tolosa, S. Go..., 252Cf  Measurement of the 252Cf source at the central position Efficiency and neutron-gamma correlations   Wed Jul 20 16:40:57 2016, S. Go, J.Agramunt, A.Tolosa, J.L. Tain,..., CLOVER  Calibration and resolution check CLOVER detectors were calibrated in energy with 60Co and 137Cs   Wed Jul 20 16:12:58 2016, S. Go, ..., CLOVER  Mounting of the CLOVER detectors in position CLOVER G7: right of beam   Wed Jul 20 16:07:58 2016, A.Tarifeņo, J.L. Tain, J. Agramunt, A. Tolosa, ..., 252Cf  19/Jul/2016 Scanning of the efficiency as a function of longitudinal position   Wed Jul 20 12:00:15 2016, J.L. Tain, J. Agramunt, A. Tarifeņo, A. Tolosa, ..., 252Cf  Measurement with the source at the center Listmode: 160719_BRIKEN_252Cf_009.dlt   Wed Jul 20 11:49:00 2016, J.L. Tain, J. Agramunt, R. Baeturia, A. Tarifeņo, A. Tolosa, ..., Background  18/07/2016  First background measurement overnight.   Wed Jul 20 11:40:00 2016, J.L. Tain, J. Agramunt, R. Baeturia, A. Tarifeņo, A. Tolosa, ..., 252Cf  First measurement with full 140 tube version  of the BRIKEN neutron detector   Wed Jul 20 11:16:18 2016, J.L. Tain, Electronics  Pulser settings We use two pulsers, Pulser1 for RIKEN, ORNL1 and ORNL2 tubes (7 PA)   Wed Jul 20 08:58:13 2016, J.L. Tain, I.Dillman, R. Caballero, J. Agramunt, A. Tarifeņo, A. Tolosa, ..., Electronics  Distribution of connections of tubes in preamplifiers and digitizers   Tue Jul 19 13:47:55 2016, A. Tarifeņo-Saldivia, Neutron efficiency - Scanning on Z preliminary result   We have carried out a scanning of the neutron efficiency with respect to the position along the Z-axis (AIDA and BEAM hole) of a 252Cf neutron source. A preliminary analysis is presented based on data from the online. A plot with the comparison of the simulations and experimental data is attached. The experimental results are in good agreement with the GEANT4 simulations of the studies for design of the neutron detector. The simulations for the   Tue Jul 19 11:54:03 2016, JL Tain A Tolosa R. Caballero A. Tarifeņo J. Agramunt , Photos of the AIDA insertion hole with the 3He tubes  RIKEN tubes on the AIDA side with the SHV right angle connector will protrude by ~95mm in the HYBRID configuration (with CLOVERS).  In the current AIDA DSSD configuration there are six detectors occupying 45-50mm    Tue Jul 19 04:34:57 2016, JL Tain A Tolosa R. Caballero A. Tarifeņo J. Agramunt , Photos of the electronics 9x Racks, crates, rear part of the preamps and matrix with all tubes.   Tue Jul 19 04:09:32 2016, JL Tain A Tolosa R. Caballero A. Tarifeņo J. Agramunt , Last tube fit in the matrix!!!  The photo of great moment   Tue Jul 19 03:19:34 2016, A. Tarifeņo, I. Dillman, J. Agramunt, A. Tolosa, J.L. Tain..., Electronics  Preamplifier and signal cable testing We check all signal cables,the flat cable connector to BNC    Mon Jul 18 19:01:36 2016, J.L. Tain, 3He tubes  Adjustment of HV and PA gain We adjust the HV for each tube type and the gain of the preamplifier (PA) in order   Mon Jul 18 18:40:32 2016, A. Tarifeņo-Saldivia and J. L. Tain, 3He tubes - Testing 7x Test of individual 3He tubes The tests were done using the ATOMKI MCA and   Mon Jul 18 09:32:50 2016, Shintaro Go, HV controls  You can start applying HVs on the detectors using macro on the control-computer. If you have already signed in the computer that controls mpod, 1. Type http://192.168.13.239/  to monitor the status of HV.   Fri Jul 15 11:47:31 2016, Nathan Brewer and Alvaro Tolosa, Preliminary Ge Calibration, Resolution and Configuration 9x Today several tests (3) were done with the germanium detectors with the voltage configuration listed in the previous entry. The tests were as follows: Tests with 60Co+137Cs sources   Fri Jul 15 08:29:14 2016, Nathan Brewer, Shintaro Go, Expected Performance and Voltage Setting for Germanium  Expected Resolution: ------------------------------ G7 should be ~2.0 keV FWHM at 600 keV for all crystals.   Sat Jul 9 21:26:25 2016, J.L. Tain, EDACQ  Electronics and DACQ for July 2016 assembly: hardware and connections   Sat Jul 9 21:21:38 2016, J.L. Tain, 3He tubes  Tube distribution in the moderator, pre-amplifiers and digitizers   Sat Jul 9 21:14:12 2016, J.L. Tain, 3He tubes  Drawings and specs of 3He tubes   Sat Jul 9 21:08:08 2016, J.L. Tain, Neutron moderator  Drawings of the polyethylene neutron moderator and table assembly   Sat Jul 9 21:00:54 2016, J.L. Tain, Hardware  A list of the available hardware   Sat Jul 9 20:44:31 2016, J.L. Tain, BRIKEN neutron detector  START Assembly and commissioning of BRIKEN neutron detector    Mon May 11 09:14:54 2015, G. Kiss, 252Cf_data_sheet  The activity of the 252Cf source, used for the calibration was 3.7 MBq at 15.05.2006. Unfortunately, uncertainty is missing from the data sheet :-(   Fri May 8 03:20:48 2015, J.Agramunt J.L.Tain K.Gabor, BnCorrelation  We run all the night until the end of beam time, and the Bn correlations are more clear now.   Thu May 7 08:36:56 2015, J.L. Tain, J. Agramunt, A. Estrade, G.Kiss, T. Davinson, C.Griffin, First BRIKEN_v.0 beta-delayed neutron correlations?  During the 98,100Kr setting run we observe  in the time correlation plot (middle right panel) of beta signals (marked by AIDA, with amplitude larger than ch=600)   Wed May 6 11:41:24 2015, J. Agramunt, A. Estrade, First online combined analysis  Screen shot of the rudimentary on-line analysis of the combined data: BRIKEN-AIDA-BigRIPS   Wed May 6 05:10:14 2015, J.L. Tain, J. Agramunt, G. Kiss, 94Se setting measurement  After the long shutdown the beam is back at 00:30 (06/05) Intensity is slightly lower 26pnA and somewhat unstable (short time) Measurement in the morning:   Wed May 6 04:57:24 2015, J.L. Tain, J. Agramunt, G. Kiss, New degrader thickness  The Al degrader thickness was reduced to 4.8mm   Tue May 5 05:29:26 2015, J.L. Tain, J. Agramunt, G. Kiss, Ambient background measurement  Beam still down. New background measurement with new RIKEN tube below the MUSIC chamber  (call it B)   Tue May 5 05:17:36 2015, J.L. Tain, J. Agramunt, G. Kiss, Ambient background measurement  Failure of a quadrupole triplet at BigRIPS (some time after earthquake) We take the chance of measuring background: File: 150504_1500_2047_bckg.root Rate per tube (n/s): U=0.098, D=0.0062, US=0.0200 Ratio to 1st 110Zr: U=1.38,  D=1.99,  US=0.90 Notes: -Compared to the 1st background measurement there are changes larger than expected statistical fluctuations:  perhaps due to slight changes in noise   Tue May 5 05:04:00 2015, J.L. Tain, J. Agramunt, G. Kiss, Change of degrader thickness  For EURICA measurements degrader thickness were increased trying to decrease MACI and AIDA trigger rate Before we had 5.7 mm of Al   Tue May 5 02:19:58 2015, j.Agramunt J.L.Tain K.Gabor , The Lower polyethylene pieces was swamped  The Lower polyethylene pieces was swamped. In the photo beam comes from the left.     Mon May 4 15:03:47 2015, J.Agramunt J.L.Tain K.Gabor , New detector placed under the beam line   New detector placed under the beam line, below MUSIC chamber This detector replace the USA tubes in the DACQ because we need the preamp to plug it.     Mon May 4 04:14:18 2015, J.Agramunt J.L.Tain K.Gabor, AIDA trigger plugged in Mod2 Ch12  AIDA trigger plugged in Mod2 Ch12   Mon May 4 03:20:00 2015, Shunji Nishimura, RNC New Rule  We have some new rule about the data taken at RNC from this year.  Shunji     Mon May 4 02:36:16 2015, J.Agramunt J.L.Tain K.Gabor, Maki trigger plugged in Mod2 Ch9      Mon May 4 02:26:14 2015, J.Agramunt J.L.Tain K.Gabor, F11 trigger plugged in Mod2 Ch16 of Briken daq      Sun May 3 10:10:13 2015, J.L. Tain, J. Agramunt, G. Kiss, 94Se setting measurement  94Se setting: File: 150503_1500_1554_94Se.root Rate per tube (n/s): U=0.966, D=0.263, US=0.538   Sun May 3 10:07:25 2015, J.L. Tain, J. Agramunt, G. Kiss, Photos of new PE shielding  Photos of the general arrangement and details of the new PE blocks   Sun May 3 09:04:07 2015, J.L. Tain, J. Agramunt, G. Kiss, Summary of neutron measurements   U: (Up: 2 RIKEN tubes at 40cm from AIDA) D: (Down: 12 RIKEN tubes at 80cm from AIDA)   Sat May 2 19:32:08 2015, AE, transfer data AIDA->BRIKEN  A test program for online data transfer is available in aidas1 PC at: /homes/npg/aev/AIDAbriken/AIDA-jorge-san.exe   Sat May 2 03:52:14 2015, J.L. Tain, 3He tube description  3He tube drawings and technical details:  RIKEN, UPC, GSI, ORNL-1, ORNL-2   Mon Apr 27 10:18:21 2015, K.Gabor S.Nishimura J.Agramunt, ORNL 3He tube at RIKEN      Mon Apr 27 04:40:43 2015, G. Kiss, J. Agramunt, neutron background at Eurica  Based on an about 8h long background measurement, the neutron background at the Eurica site was found to be about 0.006 neutron / sec (in the Riken tubes) and 0.019 neutron / sec (in the ORNL tubes). The beam was OFF.   Sat Apr 25 08:25:42 2015, G. Kiss, J. Agramunt, BRIKEN Test setup  Altogether 16  tubes are mounted for the parasitic detector test (see the attached photos): - two tubes (belonging to RIKEN) are in a 10 cm x 10 cm x 30 cm polyethylene matrix inside Eurica, the distance from AIDA is about 30 cm - 12 tubes (belonging to RIKEN) are in a 20 xm x 30 xm x 30 cm matrix, outside (below) Eurica, at the closest possible place to AIDA, the distance   Wed Feb 25 07:38:42 2015, A. Estrade J. Agramunt , Usage of synchronization test programs  In order to access to the synchronization test, we prepare two programs in the PC  briken1 ( 10.32.6.54). To Launch the processes, in a terminal type: DataSink -i 3 In other terminal type SynCheck   Tue Feb 24 09:34:54 2015, J. Agramunt, H. Baba, A. Estrade, [DAQ] DAQ correlation test   We have performed a successful test of the integration of independent DAQ systems based on a correlation  scalar counted from a common clock signal. The principles of the integration method are described in the    Mon Feb 16 00:29:00 2015, Gabor KISS, Polyethyelene  The polyethelene arrived at RIKEN. Except 4 neighboring holes (located at the inner ring) the alignment is OK.   Fri Oct 31 12:58:49 2014, Robert Grzywacz, Entry test - preamps   Here is a picture of one of our Mesytec preamplifiers. We have  located all seven of them.  They  have 16 input channels and a common SHV per board.   Fri Oct 31 11:36:57 2014, Alfredo Estrade, BRIKEN elog: take 2  A elog for the setup of the BRIKEN detector is now operational at https://elog.ph.ed.ac.uk/BRIKEN/ We have setup a list of emails that will receive automatic updates for each new entry to the logbook: C. Domingo, G. Lorusso, T. Davinson, A. Estrade, K. Rykaczewski, J.L. Tain, C. Griffin,   Fri Oct 31 09:47:59 2014, Alfredo Estrade, BRIKEN elog: Hello world!  A elog for the setup of the BRIKEN detector is now operational at https://elog.ph.ed.ac.uk/BRIKEN/   We have setup a list of emails that will receive automatic updates for each new entry to the elog:   C. Domingo, G. Lorusso, T. Davinson, A. Estrade, K. Rykaczewski, J.L. Tain, C. Griffin, S. Nishimura, I. Dillman, F. Montes, J. Agramunt, G. Cortes, F. Calvino,

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