| ID |
Date |
Author |
Subject |
Text |
 |
|
3
|
Fri Nov 3 15:06:51 2017 |
Claudia | Measurement Schedule updated | |
|
|
5
|
Fri Jul 3 14:01:38 2020 |
Claudia | Link to Ruchi's list of runs + description | https://docs.google.com/spreadsheets/d/1W1T2rC10UtOtrAaT8-ZAKFvX70v2PwDk_4-goYL-brI/edit?usp=sharing |
|
|
30
|
Thu Jun 29 09:21:13 2023 |
Annie | Info on Samples | Both Au samples (20mm and 22mm) are single
mylar.
Both Si30 (22mm) and natSi (20mm) are |
|
|
29
|
Thu Jun 22 10:37:39 2023 |
Annie | Gold 22mm Sample Images | New 22mm sample compared to old 20mm sample
used at the beginning of the campaign
+ picture of dummy target in the setup. |
|
|
64
|
Thu Apr 4 09:50:36 2024 |
CLW | First Si analysis 2024 run | Au and Si29 runs normalised by proton number
show consistency (dedicated pulses, example
detector 4). Plots for tof spectra zooming |
6x |
|
26
|
Fri Jul 29 17:21:47 2022 |
Ragan | Enriched Si-30 | Attached are the pictures of enriched Si-30
metal pieces. |
|
|
41
|
Fri Jul 28 12:19:10 2023 |
Michael Donnachie | EAR2 consistency checks, PKUP BCT SILI and normalised counts | The EAR2 ratios of BCT/PKUP, BCT/SILI
and PKUP/SILI plotted for each run for samples
Si, Sinat, Au20, Au22 and Dummy. |
10x |
|
42
|
Mon Jul 31 12:00:02 2023 |
Nikolay Sosnin | EAR2 Silicon Samples | |
|
|
44
|
Mon Aug 28 12:21:09 2023 |
Michael Donnachie | EAR2 STED Calibration Parameters | Calibration parameters for each STED detector:
With function f=p0+p1*x+p2*x*x
|
8x |
|
45
|
Mon Aug 28 14:07:23 2023 |
Michael Donnachie | EAR2 Experiment vs Simulated Amplitude Spectrums | Attatched are the overlayed compton edges
for the calibrated experimental and the GEANT4
simulations. Note p1 and p2 denotes the lower |
28x |
|
40
|
Fri Jul 28 12:07:33 2023 |
Michael Donnachie | EAR2 C6D6 timeshift issues | There seems to be issues with the EAR2
C6D6 T histograms. For Au the earlier run
seems to be shifted for detector 2 compared |
|
|
46
|
Tue Aug 29 10:32:35 2023 |
Michael Donnachie | EAR1 Parasitic vs Dedicated runs | Below are the histograms of parasitic vs
dedicated runs for EAR1. Also included are
histograms with ambient background removed |
6x |
|
56
|
Wed Nov 15 13:40:50 2023 |
Claudia | Determination of neutron capture yield and related corrections | Here are all the files needed for calculation
of the yield. There is some information that
still needs to be added to the energyandyield.c |
|
|
61
|
Sat Mar 23 15:06:44 2024 |
Nick | Detector Setup - 28/29Si Campaign 2024 | Campaign started yesterday. C6D6s placed
at 9 cm distance, angle 125 degrees w.r.t
beamline. |
9x |
|
2
|
Fri Nov 3 11:22:43 2017 |
Claudia | Detector Configuration | Distance Sample to Detector: Det1: ~10.5
cm, Det2: 11 cm, Det3: 11 cm, Det4: 11 cm
|
|
|
7
|
Mon Aug 3 14:27:18 2020 |
Nikolay Sosnin | Dead-time and BG Subtraction Meeting Slides | My TTOFSort macro is located in
/afs/cern.ch/work/n/nsosnin/public/C6D6_Calibration/Calibration_Data/Calibrator.C
|
|
|
58
|
Fri Dec 1 15:34:01 2023 |
AR | Corrected BG Subtraction plots for Zn and Au | Updated plots for Zn and Au |
6x |
|
38
|
Fri Jul 21 10:45:22 2023 |
Michael Donnachie | Consistency Checks BCT PKUP comparrisons | The ratios for BCT/PKUP for Si, Au20, Au22,
Dummy, Empty and Sinat goodfellow have been
plotted. Also included is the normalised |
12x |
|
39
|
Mon Jul 24 10:32:39 2023 |
Michael Donnachie | Consistency Checks BCT PKUP SILI | The EAR1 ratios of BCT/PKUP, BCT/SILI and
PKUP/SILI plotted for each run for samples
Si, Sinat goodfellow, Au20, Au22, Empty and |
6x |
|
53
|
Mon Nov 6 11:13:11 2023 |
Emma Walker | Comparison of empty, ambient and sample- Si-30 | Below are graphs for each sample (weighted)
showing the comparison between ambient spectra,
empty/dummy holder and sample spectra. |
16x |