MUST2 SAMURAI_2018 S3-LEB-LPC SUPERNEMO MUGAST EXPAND SCALP GALATRON HiCARI VELO
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Status ExpNbr Date Author Type Category Target-Source Subjectdown
Fixede768s Tue Jul 16 21:30:19 2019 Chloe FougeresOTHERGeneralLiFPACE4 fusion-evaporation
Simulated yields with beams 15N and 15O (4.7 MeV/u) on target LiF.
Attachment 1: fusion_evaporation_7Li.png
fusion_evaporation_7Li.png
Attachment 2: fusion_evaporation_19F.png
fusion_evaporation_19F.png
Fixede744s Mon Apr 8 14:41:07 2019 Daniele MOTHERGeneralN/APACE4 cross check ------ E744s to-do list , proposal and other relevant documents
Fusion-evaporation calculation cross-check:

angular range [10-40]deg

expected protons: ~8 pps
expected alphas: ~12 pps
expected gammas: ~90 pps


relevant output of PACE4 for 10kevents follows

************ Fusion xsection taken from Bass model
Bass fusion xsection for E = 105.0 MeV is 765 mb
Fusion radius = 4.35 fm. Barrier height is 8.06 MeV
Transmission probability for a one-dimens.barrier: Quantum-Mechanical
h_omega (curvature parameter) = 3.0 MeV

---------------------------------------------------------------------------
Starting conditions
Z N A Spin
Projectile 8 6 14 0.0
Target 6 6 12 0.0
Compound nucleus 14 12 26

Bombarding energy (MeV) 105.00
Center of mass energy (MeV) 48.46
Compound nucleus excitation energy (MeV) 63.614
Q-value of reaction (MeV) 15.152
Compound nucleus recoil energy (MeV) 56.538
Compound nucleus recoil velocity (cm/ns) 2.050e+00
Compound nucleus velocity/c 6.833e-02
Beam velocity (cm/ns) 3.807e+00
Beam velocity/c 1.269e-01

Experimental fusion cross section (mb) 765
Yrast spin at maximum excitation energy 20
Compound nucleus formation cross section (mb) 765

------ Output results for compound nucleus decay -----



1.Yields of residual nuclei

Z N A events percent x-section(mb)
14 12 26 Si 3 0.03% 0.229
14 11 25 Si 1 0.01% 0.0765
14 10 24 Si 1 0.01% 0.0765
13 11 24 Al 5 0.05% 0.382
12 12 24 Mg 16 0.16% 1.22
13 10 23 Al 29 0.29% 2.22
12 11 23 Mg 506 5.06% 38.7
11 12 23 Na 225 2.25% 17.2
12 10 22 Mg 19 0.19% 1.45
11 11 22 Na 567 5.67% 43.4
10 12 22 Ne 115 1.15% 8.79
12 9 21 Mg 8 0.08% 0.612
11 10 21 Na 139 1.39% 10.6
10 11 21 Ne 234 2.34% 17.9
11 9 20 Na 27 0.27% 2.06
10 10 20 Ne 1791 17.9% 137
10 9 19 Ne 264 2.64% 20.2
9 10 19 F 332 3.32% 25.4
10 8 18 Ne 15 0.15% 1.15
9 9 18 F 7 0.07% 0.535
8 10 18 O 2 0.02% 0.153
10 7 17 Ne 3 0.03% 0.229
9 8 17 F 354 3.54% 27.1
8 9 17 O 3 0.03% 0.229
8 8 16 O 3792 37.9% 290
8 7 15 O 123 1.23% 9.41
7 8 15 N 700 7% 53.5
8 6 14 O 17 0.17% 1.3
7 6 13 N 210 2.1% 16.1
6 6 12 C 422 4.22% 32.3
5 6 11 B 4 0.04% 0.306
5 4 9 B 65 0.65% 4.97
Total fission 1 0.01% 0.0765
TOTAL 10000 100% 765

Proton spectra in laboratory coordinates 21526 events
=============================================================================================================================
| Energy range |_________________________________________ Angular range (deg)_______________________________________________|
| (MeV) | 0 | 10 | 20 | 30 | 40 | 50 | 60 | 70 | 80 | 90 | 100 | 110 | 120 | 130 | 140 | 150 | 160 | 170 |
| | 10 | 20 | 30 | 40 | 50 | 60 | 70 | 80 | 90 | 100 | 110 | 120 | 130 | 140 | 150 | 160 | 170 | 180 |
|--------------|------|-----|-----|-----|-----|-----|-----|-----|-----|-----|-----|-----|-----|-----|-----|-----|-----|-----|
| 0.0-1.0 | 2| | 7| 13| 25| 33| 50| 71| 78| 88| 79| 64| 71| 37| 34| 33| 14| 5|
| 1.0-2.0 | | | 3| 10| 29| 73| 112| 131| 163| 158| 142| 108| 90| 71| 56| 39| 25| 13|
| 2.0-3.0 | | 3| 4| 22| 60| 110| 155| 171| 152| 163| 111| 93| 83| 56| 59| 41| 20| 6|
| 3.0-4.0 | 2| | 12| 47| 99| 174| 190| 181| 147| 120| 114| 85| 73| 60| 47| 13| 16| 7|
| 4.0-5.0 | 1| 3| 31| 68| 164| 180| 191| 171| 162| 124| 104| 63| 55| 49| 34| 24| 14| 7|
| 5.0-6.0 | 5| 24| 57| 130| 160| 196| 170| 162| 128| 94| 70| 66| 42| 31| 28| 21| 12| 4|
| 6.0-7.0 | 12| 48| 94| 151| 205| 187| 179| 139| 106| 76| 66| 61| 39| 28| 25| 14| 7| |
| 7.0-8.0 | 22| 70| 154| 184| 181| 161| 161| 137| 92| 60| 52| 35| 32| 25| 20| 14| 5| 1|
| 8.0-9.0 | 21| 94| 166| 190| 189| 179| 130| 115| 78| 49| 39| 33| 20| 18| 15| 9| 7| 1|
| 9.0-10.0 | 32| 101| 150| 171| 168| 133| 134| 79| 69| 54| 36| 24| 18| 13| 7| 4| 4| 2|
| 10.0-11.0 | 32| 105| 149| 157| 168| 138| 103| 94| 52| 42| 25| 16| 19| 9| 8| 10| 4| 1|
| 11.0-12.0 | 33| 94| 123| 156| 143| 106| 93| 63| 47| 36| 17| 15| 6| 7| 6| 2| 1| |
| 12.0-13.0 | 50| 72| 146| 151| 131| 126| 78| 64| 36| 24| 14| 11| 7| 3| 3| 1| | |
| 13.0-14.0 | 35| 89| 127| 123| 138| 103| 65| 48| 37| 19| 16| 5| 6| 2| | | | |
| 14.0-15.0 | 30| 94| 136| 116| 102| 82| 67| 47| 23| 23| 9| 6| 2| | | | | |
| 15.0-16.0 | 34| 73| 100| 103| 103| 67| 47| 32| 20| 12| 6| 2| | | | | | |
| 16.0-17.0 | 26| 92| 113| 92| 65| 66| 34| 30| 23| 11| 1| | 1| | | | | |
| 17.0-18.0 | 22| 65| 89| 83| 53| 49| 26| 14| 11| 9| 4| | | | | | | |
| 18.0-19.0 | 23| 57| 73| 81| 58| 47| 35| 17| 11| 4| | | | | | | | |
| 19.0-20.0 | 32| 72| 71| 68| 57| 43| 18| 12| 7| 4| | | | | | | | |
| 20.0-21.0 | 15| 58| 59| 43| 50| 30| 17| 7| 5| 1| | | | | | | | |
| 21.0-22.0 | 24| 39| 54| 47| 44| 29| 12| 7| 5| | | | | | | | | |
| 22.0-23.0 | 17| 38| 40| 40| 33| 18| 9| 6| 4| | | | | | | | | |
| 23.0-24.0 | 16| 42| 40| 45| 18| 14| 9| 8| | | | | | | | | | |
| 24.0-25.0 | 9| 35| 32| 27| 22| 14| 4| | | | | | | | | | | |
| 25.0-26.0 | 11| 33| 33| 22| 14| 11| 4| 1| | | | | | | | | | |
| 26.0-27.0 | 16| 20| 26| 18| 16| 8| 3| | | | | | | | | | | |
| 27.0-28.0 | 6| 26| 23| 17| 10| 6| 4| | | | | | | | | | | |
| 28.0-29.0 | 7| 19| 20| 18| 10| 5| | | | | | | | | | | | |
| 29.0-30.0 | 8| 18| 12| 13| 6| 4| | | | | | | | | | | | |
| Above 30.0 | 24| 50| 58| 40| 20| 2| | | | | | | | | | | | |
|--------------|------|-----|-----|-----|-----|-----|-----|-----|-----|-----|-----|-----|-----|-----|-----|-----|-----|-----|
| Total | 567| 1534| 2202| 2446| 2541| 2394| 2100| 1807| 1456| 1171| 905| 687| 564| 409| 342| 225| 129| 47|
| dSig/dOmega | 5e+02|4e+02|4e+02|3e+02|3e+02|2e+02|2e+02|1e+02|1e+02|8e+01|7e+01|5e+01|5e+01|4e+01|4e+01|4e+01|3e+01|4e+01|
=============================================================================================================================
| 0.0 - 5.0 | 5| 6| 57| 160| 377| 570| 698| 725| 702| 653| 550| 413| 372| 273| 230| 150| 89| 38|
| 5.0 - 10.0 | 92| 337| 621| 826| 903| 856| 774| 632| 473| 333| 263| 219| 151| 115| 95| 62| 35| 8|
| 10.0 - 20.0 | 317| 813| 1127| 1130| 1018| 827| 566| 421| 267| 184| 92| 55| 41| 21| 17| 13| 5| 1|
| Above 20.0 | 153| 378| 397| 330| 243| 141| 62| 29| 14| 1| | | | | | | | |
=============================================================================================================================


Alpha spectra in laboratory coordinates 15084 events
=============================================================================================================================
| Energy range |_________________________________________ Angular range (deg)_______________________________________________|
| (MeV) | 0 | 10 | 20 | 30 | 40 | 50 | 60 | 70 | 80 | 90 | 100 | 110 | 120 | 130 | 140 | 150 | 160 | 170 |
| | 10 | 20 | 30 | 40 | 50 | 60 | 70 | 80 | 90 | 100 | 110 | 120 | 130 | 140 | 150 | 160 | 170 | 180 |
|--------------|------|-----|-----|-----|-----|-----|-----|-----|-----|-----|-----|-----|-----|-----|-----|-----|-----|-----|
| 0.0-1.0 | 2| 17| 19| 35| 40| 38| 31| 28| 22| 35| 16| 17| 16| 10| 13| 5| 1| |
| 1.0-2.0 | 13| 35| 55| 71| 59| 70| 61| 42| 36| 35| 20| 18| 17| 16| 9| 5| 6| 1|
| 2.0-3.0 | 17| 33| 65| 90| 77| 80| 47| 39| 42| 29| 19| 18| 18| 12| 5| 1| 2| 1|
| 3.0-4.0 | 9| 37| 58| 109| 103| 82| 60| 34| 32| 26| 8| 18| 9| 5| 5| 1| | 1|
| 4.0-5.0 | 12| 33| 69| 128| 102| 57| 58| 34| 24| 23| 17| 5| 8| 4| 2| 1| 1| |
| 5.0-6.0 | 4| 41| 77| 112| 118| 78| 60| 40| 24| 19| 1| 4| 4| 1| 2| | 1| 1|
| 6.0-7.0 | 2| 25| 91| 135| 116| 100| 50| 30| 21| 10| 8| 5| 5| | 1| 1| | |
| 7.0-8.0 | 3| 30| 83| 132| 139| 90| 42| 27| 13| 8| 9| 4| 2| | | | | |
| 8.0-9.0 | 3| 40| 89| 149| 105| 70| 35| 20| 14| 5| 1| 2| 1| 1| | | | |
| 9.0-10.0 | 2| 32| 115| 137| 123| 61| 33| 12| 15| 5| 1| 3| 1| | | | | |
| 10.0-11.0 | 7| 39| 124| 143| 105| 61| 27| 20| 11| 2| 1| | | | | | | |
| 11.0-12.0 | 8| 48| 119| 130| 93| 64| 23| 17| 11| 5| | | | | | | | |
| 12.0-13.0 | 14| 57| 138| 138| 83| 52| 26| 10| 8| 1| | 1| | | | | | |
| 13.0-14.0 | 12| 67| 142| 121| 89| 38| 20| 12| 6| | | | | | | | | |
| 14.0-15.0 | 15| 79| 130| 124| 77| 34| 24| 12| 6| | | | | | | | | |
| 15.0-16.0 | 25| 80| 158| 117| 68| 44| 18| 9| 2| 2| | | | | | | | |
| 16.0-17.0 | 27| 104| 143| 119| 53| 26| 11| 8| 2| 1| 1| | | | | | | |
| 17.0-18.0 | 36| 97| 129| 109| 65| 27| 19| 6| 2| 2| | | | | | | | |
| 18.0-19.0 | 32| 103| 140| 101| 55| 23| 8| 8| 2| 1| | | | | | | | |
| 19.0-20.0 | 39| 110| 120| 79| 54| 29| 10| 4| 1| | | | | | | | | |
| 20.0-21.0 | 44| 118| 118| 55| 30| 22| 9| 2| | | | | | | | | | |
| 21.0-22.0 | 35| 98| 101| 69| 29| 13| 7| 2| 1| | | | | | | | | |
| 22.0-23.0 | 36| 83| 95| 67| 26| 11| 6| 2| 2| | | | | | | | | |
| 23.0-24.0 | 48| 77| 90| 49| 31| 4| 7| 3| | | | | | | | | | |
| 24.0-25.0 | 35| 85| 60| 51| 22| 15| | 1| 1| | | | | | | | | |
| 25.0-26.0 | 46| 84| 75| 42| 28| 12| 7| 1| | | | | | | | | | |
| 26.0-27.0 | 41| 74| 87| 42| 29| 7| 4| | | | | | | | | | | |
| 27.0-28.0 | 39| 59| 46| 44| 26| 3| 3| | | | | | | | | | | |
| 28.0-29.0 | 27| 66| 63| 32| 21| 6| 4| | | | | | | | | | | |
| 29.0-30.0 | 33| 64| 39| 31| 13| 9| | | | | | | | | | | | |
| Above 30.0 | 335| 592| 401| 226| 91| 18| 2| 1| | | | | | | | | | |
|--------------|------|-----|-----|-----|-----|-----|-----|-----|-----|-----|-----|-----|-----|-----|-----|-----|-----|-----|
| Total | 1001| 2507| 3239| 2987| 2070| 1244| 712| 424| 298| 209| 102| 95| 81| 49| 37| 14| 11| 4|
| dSig/dOmega | 8e+02|7e+02|5e+02|4e+02|2e+02|1e+02|5e+01|3e+01|2e+01|1e+01| 7| 7| 7| 5| 4| 2| 3| 3|
=============================================================================================================================
| 0.0 - 5.0 | 53| 155| 266| 433| 381| 327| 257| 177| 156| 148| 80| 76| 68| 47| 34| 13| 10| 3|
| 5.0 - 10.0 | 14| 168| 455| 665| 601| 399| 220| 129| 87| 47| 20| 18| 13| 2| 3| 1| 1| 1|
| 10.0 - 20.0 | 215| 784| 1343| 1181| 742| 398| 186| 106| 51| 14| 2| 1| | | | | | |
| Above 20.0 | 719| 1400| 1175| 708| 346| 120| 49| 12| 4| | | | | | | | | |
=============================================================================================================================

Gamma ray spectrum 71373 events

Emission from unbound and bound states(*), and total gamma ray spectrum
(*) note that emission of a particle from an unbound state is not allowed in the code if Ecm is less than Emin

=======================================================================================
| Energy range (MeV) | Unbound | Bound | TOTAL |
|------------------------------------|------------------|---------------|-------------|
| 0.0 - 1.0 | 11 | 4104 | 4115 |
| 1.0 - 2.0 | 23156 | 44070 | 67226 |
| 2.0 - 3.0 | 3 | 0 | 3 |
| 3.0 - 4.0 | 1 | 0 | 1 |
| 4.0 - 5.0 | 4 | 0 | 4 |
| 5.0 - 6.0 | 4 | 0 | 4 |
| 7.0 - 8.0 | 4 | 0 | 4 |
| 8.0 - 9.0 | 4 | 0 | 4 |
| 9.0 - 10.0 | 1 | 0 | 1 |
| 10.0 - 11.0 | 3 | 0 | 3 |
| 11.0 - 12.0 | 4 | 0 | 4 |
| 12.0 - 13.0 | 1 | 0 | 1 |
| 13.0 - 14.0 | 3 | 0 | 3 |
|------------------------------------|------------------|---------------|-------------|
| Total | 23199 | 48174 | 71373 |



iulian wrote:
To do list
Monday
- ask final beam energy for the 14O beam (include CATS removal)-> E=7.50 MeV/u
- Mount CATS timing (much thinner) at Cats1 position
- make a hole target, diameter = 7 mm, thick target (Al?)
- dismount targets with gloves due to the contamination
- mount targets (list ..… + hole target)
Target list ( Hole Target, 200 um CH2 (?), 100 um CH2, C target, 100 um CH2, 70 um CH2 )
- remove the Vamos entrance DCs
- install the VAMOS finger, larger one
- Id plots with Vamos
- to mount / or not a MCP
- Prepare Agata Or - HFpropre and Agata 52 – HFpropre for beam intensity monitoring.
- Solve the MM3 EY problems (see previous elog entry)
- Understand Vamos (40% efficency) and Agata efficiency (5% efficiency Agata instead of 10%) for 2H(16O,p)17O
- Make an acq run with Mugast in air to understand if detectors contaminated

You will find:
E744s.pdf last infos about E744
Proposal__15F_6.pdf the proposal as it was for 2018 Lise run
time_request_E744.pdf time request for Vamos-Agata run
Fixedcom2019 Fri Apr 5 19:42:28 2019 Jenn Sanchez & Ana Montaner-PizáOTHERGeneralCD2PACE4 calculations

Attached you can find the PACE4 calculations for the reactions 16O + 12C and 16O + d at 6 MeV/u beam.

Main cross sections are:
* 25Mg (232 mb, 25%) and 16O (182, 21%) (for 16O+12C).
* 17O (292 mb, 42%) and 14N (270, 39%) (for 16O+d).





Attachment 1: 16O_12C.png
16O_12C.png
Attachment 2: 16O_d.png
16O_d.png
Fixede768s Tue Jul 16 22:25:51 2019 mugastOTHERGeneral Oxygen 15 decay scheme
beta+ decay to the ground state of 15N
gammas @ 511 keV
Attachment 1: 15O_decay_scheme.png
15O_decay_scheme.png
PendingTEST Tue Jan 21 17:55:12 2020 MarlèneMUST2Hardware Ovv error on the -5V of CAEN boards
The Ovv error shows on the -5V (first one) of the 3 board (5,3.3,10V for MUST2§squares)
It means that the voltage is over the asked value.
If we ask 5V, we get 5.5V in reality

We changed for 4.5V and we get 5V. The current is different from the one on the MUGAST BT box but we don't know how many detectors are connected.
We exchanged cables and found the same current in the other board, so we guess that it is still working properly.
A check of stability should be done.
Attachment 1: BT_referenve_5V_cables_inv_a_comp_referenve_5V_partMUST2
Attachment 2: BT_referenve_5V_partMUST2_cables_inv_a_comp_referenve_5V
Attachment 3: BT_referenve_5V_partMUST2
Attachment 4: BT_referenve_5V
Fixede768s Fri Jul 19 08:09:21 2019 Jenn, KseniiaOTHERGeneral Overview nightshift run 112
Smooth night, everything was working properly.
Checked agata rootfile to see preliminary gammas.

19Ne 275 state observed

Also 19F (strong 109 state) (fusion-evaporation?)

Check Agata elog for more details.
Fixedcom2019 Sun Apr 7 21:35:51 2019 Valerian, Freddy and AntoineRUNGeneralN/AOvernight run259 crashed during the night
Run 259 which was an overnight run crashed (During the night between the 6 and the 7th of April).

The result of this crash was that the the acquisition started writing a 4gb file each seconds for 80 seconds. We then had to remove the run (~300gb) as the quota allowed by GANIL to the mugast account was reached.
We also transfered the output of the Nptool analysis to the /data/evamosX/com2019/Analysis/nptool_outputs/ and made a symbolic link to this folder in the nptool/Output in order not to ever reach the quota again (Antoine seems to have no quota, or at least multiple Pb of quota...)
Fixede744s Mon Apr 15 15:18:55 2019 A. LemassonVAMOSHardware Optimization of IC Shaping
During Run 129,
1) investigation of the trapezoidal filter of IC
2) The Conclusion is that if we reduce the shaping to 2.5 us we reduce the random line in IC vs IC (At 1e5 in VAMOS : Random Line / Peak is 18.5 % compared to 40% for shaping of 3us)
3) The 2.5us us also optimum for the resolution (oscillation of the abse line after the filter very sensitive to K, with freq of ~500Khz)

/!\ Increasing intensity during the study


Flat Top 1.07 , 320ns k+0.5M

K sigma
0.5 81 530
1.0 236 1038 0.53
1.5 161 1549 0.25
2. 215 2039 0.247
2.5 156 2554 0.1435
3. 260 3082 0.196

Changing N
320 2.5 126 2554 0.116
160 2.5 126 2554 0.116
40 2.5 130 2554 0.119

Chnging Q
2980 40 2.5 130 2554 0.1119
3300 40 2.5 134 2554 0.123

Chnging M

1070 3300 40 2.5 134 2554 0.123
500 2900 40 2.5 145 2554 0.133
750 3000 40 2.5 145 2554 0.133


-> Final Setting is
M Q N K
1070 3200 160 2.5 -> 126/2554 -> 0.116
Attachment 1: IC_Shapingafter_run129.png
IC_Shapingafter_run129.png
Fixede744s Tue Apr 16 00:01:43 2019 louis, GuiseppeONLINEGeneralCH2Online snapshot from run 132
Online snapshot from run 132
Attachment 1: run131_Mugast_28.png
run131_Mugast_28.png
Attachment 2: run131_Mugast_27.png
run131_Mugast_27.png
Attachment 3: run131_Mugast_26.png
run131_Mugast_26.png
Attachment 4: run131_Mugast_25.png
run131_Mugast_25.png
Attachment 5: run131_Mugast_24.png
run131_Mugast_24.png
Attachment 6: run131_Mugast_23.png
run131_Mugast_23.png
Attachment 7: run131_Mugast_22.png
run131_Mugast_22.png
Attachment 8: run131_Mugast_21.png
run131_Mugast_21.png
Attachment 9: run131_Mugast_20.png
run131_Mugast_20.png
Attachment 10: run131_Mugast_19.png
run131_Mugast_19.png
Attachment 11: run131_Mugast_18.png
run131_Mugast_18.png
Attachment 12: run131_Mugast_17.png
run131_Mugast_17.png
Attachment 13: run131_Mugast_16.png
run131_Mugast_16.png
Attachment 14: run131_Mugast_15.png
run131_Mugast_15.png
Attachment 15: run131_Mugast_14.png
run131_Mugast_14.png
Attachment 16: run131_Mugast_13.png
run131_Mugast_13.png
Attachment 17: run131_Mugast_12.png
run131_Mugast_12.png
Attachment 18: run131_Mugast_11.png
run131_Mugast_11.png
Attachment 19: run131_Mugast_10.png
run131_Mugast_10.png
Attachment 20: run131_Mugast_9.png
run131_Mugast_9.png
Fixedcom2019 Sat Apr 6 02:48:39 2019 Iulian RuxandraRUNSoftware Online Spectra run 256 @2h30 am 06/04 (for reference)
The online spectra (for reference)
No timing on Mg3 & Mg4 side X. Those correspond with the masked channels on the Muvi1
Attachment 1: Run_256_Impact_Matrix.png
Run_256_Impact_Matrix.png
Attachment 2: Run_256_Must_X_side.png
Run_256_Must_X_side.png
Attachment 3: Run_256_TACs.png
Run_256_TACs.png
Attachment 4: Run_256_Must_Y_side.png
Run_256_Must_Y_side.png
Attachment 5: Run_256_Must_X_side.png
Run_256_Must_X_side.png
Attachment 6: Run_256_Impact_Matrix.png
Run_256_Impact_Matrix.png
Attachment 7: Run_256_Vamos_1.png
Run_256_Vamos_1.png
Attachment 8: Run_256_Vamos_2.png
Run_256_Vamos_2.png
Attachment 9: Run_256_Vamos_3.png
Run_256_Vamos_3.png
Attachment 10: Run_256_Vamos_4.png
Run_256_Vamos_4.png
Attachment 11: Run_256_Vamos_5.png
Run_256_Vamos_5.png
Fixedcom2019 Sat Apr 6 08:18:55 2019 mugastRUNSoftwareCD2Online Scalers run 256 @8h00 am 06/04 for reference
Attachment 1: Scalers060419-08am.png
Scalers060419-08am.png
Attachment 2: Must2X060419-08am.png
Must2X060419-08am.png
Attachment 3: Must2Y-060419_08am.png
Must2Y-060419_08am.png
Attachment 4: Must2MugastXYMatrix060419_08am.png
Must2MugastXYMatrix060419_08am.png
Attachment 5: MUGAST060419_08am.png
MUGAST060419_08am.png
Fixedcom2019 Sat Apr 6 02:52:51 2019 Iulian RuxandraRUNSoftware Online Scalers run 256 @2h30 am 06/04 for reference
Attachment 1: Run_256_Scaler1.png
Run_256_Scaler1.png
Attachment 2: Run_256_Scaler2.png
Run_256_Scaler2.png
Attachment 3: Run_256_Scaler3.png
Run_256_Scaler3.png
Attachment 4: Run_256_Scaler4.png
Run_256_Scaler4.png
Fixede786s Wed Jun 12 17:59:01 2019 mugastOTHERSoftware Online Energy Calibration
Updated Online Energy calibration for MUGAST, based on run_0231 data
Attachment 1: x_E_cal.png
x_E_cal.png
Attachment 2: y_E_cal2.png
y_E_cal2.png
Fixede786s Wed Jun 12 18:11:04 2019 mugastOTHERSoftware Online Energy Calibration
Fixede793s Fri Mar 12 09:52:01 2021 mugast (Sarah, Louis)OFFLINEGeneralCD2Offline analysis run up to 56 8am
1) A high energy gamma has been identified at 3505 keV by gating on 3-5 MeV range in excitation energy. This transition is unknown so far

2) preliminary angular distribution has been extracted for the p states(<1MeV) and the f states (3-5MeV) corrected from geometrical efficiency. Angular distribution with gate on the 3.5 MeV gamma was also extracted. Too few statistics to tell anything. Need at least 4 time more statistics to have a proper angular distribution.
Attachment 1: AngDisrtib.png
AngDisrtib.png
Attachment 2: 3MeV_gamma.png
3MeV_gamma.png
Attachment 3: AWBA.png
AWBA.png
Fixede786s Wed Jun 26 05:58:23 2019 FreddyOFFLINEGeneralN/AOffline analysis run 56 and 58
Attachment 1: run56-58_analysis.png
run56-58_analysis.png
Attachment 2: run56-59_analysis_gammarays.png
run56-59_analysis_gammarays.png
Attachment 3: run56_analysis.png
run56_analysis.png
Attachment 4: run58_analysis.png
run58_analysis.png
Fixede786s Tue Jun 25 02:46:32 2019 Sylvain, LouisOFFLINEGeneralCryo-3HeOffline analysis run 56
Offline analysis of run 56 has been perfomed. On plots, kinematics lines and excitation energy are shown using gate on 47K in vamos. Then agata spectra is shown using gate on 47K in VAMOS un valid event in MUGAST. One can (may be) distinguish a peak at 368keV...
Attachment 1: Kine_run56.png
Kine_run56.png
Attachment 2: TripleCoinc_run56.png
TripleCoinc_run56.png
Fixede793s Sat Mar 13 10:11:44 2021 AdrienOFFLINEGeneralCD2Offline analysis of run 51-61
Run 51 to 61 are converted and analysed.
I fixed the gamma/no gamma normalisation after binning change.

We clearly see :
a state at 2.5 MeV that decay directly to the g.s. and a state at around 5 MeV with a 3 gamma cascade.

To do list:
- Add an angle dist in AngDist.C macro for the states around 2MeV (you can remove the Ex plot)
- Put Logy in all the canvas for the angle dist;)
- create a new macro showing the EDC 1D histo gated on several sliding windows in Ex to see the the gamma peak changing height
- add arrow or line indication the gamma rays position on every plots
- build the level scheme based on this (there is a preliminary scheme posted earlier by Manu based on gamma-gamma).
Attachment 1: Plot51-61.png
Plot51-61.png
Attachment 2: Angle51-61.png
Angle51-61.png
Fixede793s Wed Mar 10 22:19:22 2021 Adrien, Freddy, Wilton and NigelOFFLINEGeneralCD2Offline analysis of run 51 and 52 using ganil files
We noted that the gamma ray efficiency calculated from file converted from AGATA was close 100%. We concluded that the conversion program was reauiring a gamma ray to be present.

This is confirm by analysis of the ganil dta file that show 10 time more count that the agata one.

Here is a kinematical plot of the run 51 and 52 analysised from ganil file.

There is a 1.5MeV state present that disappear in the agata coincidence. This is to be investigated with more data. Is it an isomer state? from 48K? 48Ti?
Attachment 1: RUN5152_ELabThethaLab.png
RUN5152_ELabThethaLab.png
Fixede786s Mon Jun 24 06:14:02 2019 LouisOFFLINEGeneralCryo-3HeOffline analysis 46Ar(3He,d)47K for run 49
Energy loss vs. Time of Flight identification has been performed in mugast. On can notice some calibration trouble in energy and time. Big shift of the deToF bananas are seen from one telescope to an other. Furthermore, one can distinguish proton and deuteron in MG1, 3 and 4 but it's it's very difficult to conclude for 5,7 and 11.

From those plots, deuteron has been selected. Adding a cut on the center of the CATS profile and on the Brho in vamos, energy and angle in the laboratory has been computed. And then the excitation energy. Nothing clear for the moment...

a macro "Get46ArHe3d.C" which apply cuts and generate a new tree with only gated event is written in:
/home/mugast/analysis/nptool/Projects/MUGAST/macros/e786s
the generated tree "46ArHe3d.root" contains only event which passed cuts.

cheers
Attachment 1: Kine.png
Kine.png
Attachment 2: dEToFMG.png
dEToFMG.png

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