Fixed, e768s, Sat Jul 20 11:33:01 2019, Christian, OTHER, General, , Previous Papers - gamma decays from states in the 4-MeV region
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This search was triggered by our lack of seeing the 3958keV line at the expected level. 2689 keV line observed (runs 112,115,116) as 55-60 counts. Expected
yield in 3958 keV line based on 80:20 branching and 1.5:1.0 efficiency is 10 counts. We see (at most) 2 in the full photo-peak for this line. (Theses two
counts are also lower than expected by about 20 keV.)
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Fixed, e768s, Sat Jul 20 12:06:00 2019, Christian, OTHER, General, , Previous Papers - gamma decays from states in the 4-MeV region
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Further to the previous post on gamma-ray lines, attached is Kanungo's paper on doppler-attenuation measurement of the 4033 line for lifetime measurement.
The lower-energy lines are, however, not included in the figures. |
Fixed, e768s, Sat Jul 20 12:57:41 2019, Christian, OTHER, General, , Previous Papers - gamma decays from states in the 4-MeV region
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2019 paper by Hall, Bardayan, et al., gamma decays of 4.14 and 4.20 states, g-g-t triple coincidences.
Abstract:
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Fixed, e768s, Sat Jul 20 14:21:22 2019, Nikola, ONLINE, General, , screenshots run 117 @ 14h20 22x
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Fixed, e768s, Sat Jul 20 19:21:56 2019, Marlene, Nicolas, Christian, Fairouz, OFFLINE, General, , Trying to understand AGATA g-ray yields
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goal: we want to check whether the yields of the 1297.7 keV (from 19Ne 1536, 3/2+, l=1 state) and 1340 keV (from 19Ne 1615, 3/2-, l=2 state) g-ray lines
is compatible with what we expect from x-sec calculations
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Fixed, e768s, Sat Jul 20 23:32:44 2019, Sylvain Fairouz, OFFLINE, General, , Trying to understand AGATA g-ray yields
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[quote="Marlene, Nicolas, Christian, Fairouz"]goal: we want to check whether the yields of the 1297.7 keV (from 19Ne 1536, 3/2+, l=1 state) and 1340 keV
(from 19Ne 1615, 3/2-, l=2 state) g-ray lines is compatible with what we expect from x-sec calculations
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Fixed, e768s, Sat Jul 20 23:57:34 2019, Diego, OFFLINE, General, , VAMOS acceptance, comparison between 9+ and 10+ states
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Figures above, simulation of VAMOS acceptance for 10+ and 9+ 19Ne charge states. Ratio between them quite big (0.58)
Figures below, comparison of the states with offline data. Ratio much smaller.
It seems like acceptance doesn't cut the 10+ charge state too much, but 10+ is less produced than 9+. |
Fixed, e768s, Sun Jul 21 14:54:28 2019, Marlène, RUN, General, , run 119 scalers 
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Fixed, e768s, Sun Jul 21 16:39:38 2019, Marlène, Antoine, BEAM, General, , IMPORTANT :How to send scalers to PCP
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Go to PCP
Open a terminal
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Fixed, e768s, Sun Jul 21 16:42:20 2019, Marlène, OFFLINE, General, , Conversion of data from AGATA :update
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When VAMOS VXI crashed (run 118) the Action file was recompiled.
As AGATA conversion is not copying the ACTION file for each run, it used the old version by default (from 16th of july).
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Fixed, , Sun Jul 21 16:51:30 2019, Marlène, Christian, Ksenia, BEAM, General, , trial of tracking of the implantation of 15O
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Looking at AGATA count rate, we have seen that the highest counting rate for 511 keV line is seen in the inner ring (0*A clusters).
The outer ring detectors (10B for example) counts 10 times less.
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Fixed, e768s, Sun Jul 21 17:02:25 2019, Marlène, BEAM, General, , beam intensity in the afternoon
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Fixed, e768s, Sun Jul 21 17:45:54 2019, kseniia, AGATA, General, , Current total stats on 19Ne 
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Stats from runs 112, 115, 116, 117, 118, 119(~15h)
beta = 8%
Q = 9 & 10 |
Fixed, e768s, Sun Jul 21 17:57:08 2019, Christian, OTHER, General, , Previous Papers - gamma decays from states in the 4-MeV region
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In comment to previous entry (see thread), on the 2019 Hall paper on 19Ne transitions:
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Fixed, , Sun Jul 21 22:28:11 2019, Kseniia, AGATA, General, , 15O implantation 
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Attached is the intensity distribution of 511 keV in run 119 (first image) vs run 120 (second image).
In between the two runs, beam optics was twitched.
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Fixed, , Sun Jul 21 23:18:25 2019, Kseniia, AGATA, General, , Current total stats on 19Ne
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Runs 112, 115, 116, 117, 118, 119, 120 and ~1h of 121
We see 3 peak candidates with energies not matching anything known |
Fixed, e768s, Mon Jul 22 10:10:02 2019, Christian, OTHER, General, , Previous Papers - alpha-branching ratios for states in the 4-MeV region   
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Branching ratio data overview from Tan et al. (PRL 2007, attached):
Ex/MeV B_alpha
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Fixed, e768s, Mon Jul 22 11:21:25 2019, mugast, MUST2, Software, , Pedestals of MG3 
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Pedestals of MG3_X have changed yesterday, they are back to about 8200 as they should be --> saved in ped_muvi2sec2_22072019_new
We are using wrong pedestals (of about 9600) --> the pedestals are saved under mugast account as ped_muvi2_sec2_22072019_sameas_1807219
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Fixed, , Mon Jul 22 12:33:17 2019, Kseniia, AGATA, General, , Stats on 19Ne  
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Full stats for runs 112..124 with the event-by-event Doppler correction. So, we see 4140 kev.
Also, the betas of all the 19Ne with Q= 9,10 identified in VAMOS |
Fixed, , Mon Jul 22 12:54:25 2019, Kseniia, AGATA, General, , Beta vs gamma-ray energy in 19Ne, runs 112-124
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