AIDA GELINA BRIKEN nToF CRIB ISOLDE CIRCE nTOFCapture DESPEC DTAS EDI_PSA 179Ta CARME StellarModelling DCF K40
  nTOFCapture, Page 2 of 4  ELOG logo
  ID Date Authordown Subject
  25   Sat Mar 19 17:29:43 2022 Nikolay SosninAl26 Experimental Inventory at n_TOF

Three aluminium crates contain 26Al(n, alpha) kit from EAR2, and was in the barracks (building 6547) near detector lab by EAR1 entrance. A list is attached and photos can be found on Dropbox:

https://www.dropbox.com/sh/68k1xove2zr1bmj/AADKvN8wR_Ia2EwZMOXZqdMCa?dl=0

  33   Sat Jul 15 07:33:32 2023 Nikolay Sosnin30Si EAR2

8 sTED + 2 C6D6

C6D6: distance = 14 cm, angle = 135 degrees

sTED horizontal ring, distance for each detector from target = 4.5 cm. sTED labeled 8 in the DAQ is actually sTED #9 at n_TOF (actual sTED #8 showed no signal)

sTED1 809V, sTED2 793V, sTED3 813V, sTED4 779V, sTED5 785V, sTED6 800V, sTED7 791V, sTED8 837V

C6D61 (labeled C6D6_M in HV log) 854V, C6D62 (labeled C6D6_N in HV log) 871V

  34   Mon Jul 17 10:06:35 2023 Nikolay SosninState of the Union: Campaign Update 17.07.2023

EAR1: Si-nat sample fell off the holder during maintenance (before run 116544), appears intact and undamaged. Placed it back in-beam for further EAR1 measurements and subsequent transfer to EAR2.

EAR2: Replaced DUMMY with 30Si. Photo during alignment and photo of sample in holder attached.

  36   Mon Jul 17 12:30:28 2023 Nikolay SosninSi-nat Goodfellow Sample Properties

Goodfellow sample has been deposited on a single Mylar foil and glue is drying.

mass = 2.932 g

diameter = 20.0 mm

thickness = 3.98 mm

  37   Mon Jul 17 14:49:16 2023 Nikolay SosninMounted Si-nat Sample

Goodfellow Si-nat mounted at EAR1. First run: 116551

  42   Mon Jul 31 12:00:02 2023 Nikolay SosninEAR2 Silicon Samples
  61   Sat Mar 23 15:06:44 2024 NickDetector Setup - 28/29Si Campaign 2024

Campaign started yesterday. C6D6s placed at 9 cm distance, angle 125 degrees w.r.t beamline.

Measured calibration sources: Cs137, Y88, AmBe, CmC. Measuring Si-nat over the weekend.

Detector          Voltage

    C6D6_D_1 1550          
    C6D6_E_2 1590          
    C6D6_H_3 1460          
    C6D6_L_4 1450

 

  62   Mon Mar 25 09:07:53 2024 NickProton Monitoring

https://docs.google.com/spreadsheets/d/18lk27N6Pb2iT_xtDA-1T1c9vVubXTJ0OsaDjOxErP0I/edit?usp=sharing

  31   Thu Jul 13 12:27:44 2023 Michael Donnachie, CLWCalibration Parameters

Calibration parameters for each detector:

detector y-intercept (value) y-intercept (error) gradient (value) gradient (error)
1
3.71330E-02
5.54684E-03
2.78468E-04
1.56343E-06
2
1.21071E-02
7.19950E-03
2.82656E-04
1.96751E-06
3
2.74746E-02
4.18331E-03
2.64094E-04
1.33883E-06
4
2.96214E-02
4.61155E-03
2.73633E-04
1.22941E-06

A linear function was fitted to the reference point channel (from experimental histogram) and reference point energy (from simulation histogram). The reference point 'r' was r=mean+(FWHM/2) for a gaussian fitted to each compton edge. 

 

The comparrisons between the calibrated experimental and simulation histograms has been attached. P1 (left) and P2 (right) on the Y88 hisograms indicate whether the histograms were scaled with respect to the leftmost or rightmost compton edge (only to allow easier comparrison). 

Broadening parameters applied to the simulations

float a1 = 0.004947965;
float b1 = 0.005227974;
float a2 = 0.007163802;
float b2 = 0.007549987;
float a3 = 0.001256462;
float b3 = 0.006410511;
float a4 = 0.003907402;
float b4 = 0.004033837;

sigma= sqrt(axE+bxE^2) 

  38   Fri Jul 21 10:45:22 2023 Michael DonnachieConsistency 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 counts (counts/BCT) with all 4 detectors on one plot. Apologies there is not a legend, however det1 is red, det2 is green, det3 black and det4 blue. 'counts' for Si was integreated over the Si resonance, for Au it was integrated over the largest resonance. For Dummy, Empty and Sinat the counts were integrated over a large range of 1e+5 to 1e+7ns. The Sinat resonance was too small for adequate statistics to only integrate over the resonance hence why a large range was used. 

 

  39   Mon Jul 24 10:32:39 2023 Michael DonnachieConsistency 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 Dummy. 

  40   Fri Jul 28 12:07:33 2023 Michael DonnachieEAR2 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 to the rest. 

For Si plotted is 3 different runs 216123, 216128 and 216135 for both detectors. The histogram is messy but highlights that there is a problem. The single Si resonace should be around 20 000ns and this is only the case for run216128. 

Apologies for no legend on plots. 

Au22
det1 run216158 black
det1 run216109 red
det2 run216158 green
det2 run216109 blue

Au22
det1 run216157 black
det1 run216108 red
det2 run216157 green
det2 run216108 blue
 

  41   Fri Jul 28 12:19:10 2023 Michael DonnachieEAR2 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. 

Also included is the normalised counts (counts/BCT) with 7 detectors on one plot (STED8 was ommited).  'counts' for Si was integreated over the Si resonance, for Au it was integrated over the largest resonance. For Dummy and Sinat the counts were integrated over a large range of 1e+4 to 1e+6ns. The Sinat resonance was too small for adequate statistics to only integrate over the resonance hence why a large range was used. The C6D6 normalised counts were not plotted as there seems to be issues with this detector in EAR2. 

 

  44   Mon Aug 28 12:21:09 2023 Michael DonnachieEAR2 STED Calibration Parameters

Calibration parameters for each STED detector: With function f=p0+p1*x+p2*x*x

Detector

p0 Value  p0 Error p1 Value p1 Error p2 Value p2 Error

STED 1

5.67257E-02
1.26442E-02
2.98739E-03
7.35717E-05
5.53612E-09
6.80573E-08
STED 2
3.28429E-02
8.70646E-03
3.65244E-03
6.73960E-05
-1.00906E-07
7.35018E-08
STED 3
4.94516E-02
9.74176E-03
3.09050E-03
6.48451E-05
4.55854E-08
5.55624E-08
STED 4
5.28963E-02
9.01234E-03
3.72607E-03
7.13115E-05
8.07590E-08
7.71976E-08
STED 5
5.72747E-02
9.19542E-03
2.91606E-03
6.10110E-05
9.73475E-08
5.75051E-08
STED 6
6.56951E-02
7.56334E-03
3.15511E-03
5.22840E-05
3.41401E-08
5.06241E-08
STED 7
4.66976E-02
8.08261E-03
3.12827E-03
5.32355E-05
7.80229E-09
5.79147E-08

A quadratic function was fitted to the reference point channel (from experimental histogram) and reference point energy (from simulation histogram). The reference point 'r' was r=mean+(FWHM/2) for a gaussian fitted to each compton edge. A quadratic function was used as it fitted the higher energy AmBe reference point better than a linear function. This is highlighted by the comparisson of "STED 2 Calibration" and "STED 2 Example Linear Fit Calibration" plots below. The p0 error is quite large and p2 error very large (larger than the parameter value in STED1) - however the parameters are highly correlated which may have inflated the error. 

CmC histograms were not used as the compton edge could not be located. 

For reference the STED 1 correlation matrix:

  p0 p1 p2
p0 1 -0.92473 0.78779
p1 -0.92473 1  -0.91714
p2 0.78779 -0.91714 1

 

  45   Mon Aug 28 14:07:23 2023 Michael DonnachieEAR2 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 and higher energy compton edges for Yttrium. 

The experimental and simulated histograms are shifted in quite a few of these plots suggesting the calibration was not fully successful. The compton edge for AmBe was difficult to locate and may have contributed to the poor calibration. 

  46   Tue Aug 29 10:32:35 2023 Michael DonnachieEAR1 Parasitic vs Dedicated runs

Below are the histograms of parasitic vs dedicated runs for EAR1. Also included are histograms with ambient background removed which closes the gap between parasitic and dedicated histograms. This was preformed by scaling the ambient by counts by a multiplication of (dedicated or parasitic) bunch number/ambient bunch number. There are no legends but the dedicated counts are in black and parasitic counts in red. Only included are C6D6 1 detectors but the other three detectors were equivelant. 

 

 

  47   Wed Aug 30 12:08:45 2023 Michael DonnachieProcessing files

Here are the Processing files for EAR1 and EAR2 with calibrations.

  48   Wed Oct 18 12:14:09 2023 Emma WalkerProcessing file for EAR-1 with WF applied, Si-30

Weighting function for Si-30, Au22, Au20 and Sinatgood applied for parasitic and dedicated beams. 

  49   Mon Oct 23 12:39:33 2023 Emma WalkerSi-30 corrected weighted and dead time corrections histograms (dedicated)

Si-30:

Histograms for dead time corrections for all 4 C6D6 detectors.

Histograms for weighted and deadtime corrected dedicated spectra. 

  50   Mon Oct 23 12:47:16 2023 Emma WalkerSi-30 weighted and corrected spectra and deadtime correction histograms (parasitic)

Si-30:

Histograms for deadtime correction for all 4 C6D6 detectors for parasitic beam.

Histograms for weighted and deadtime corrected parasitic spectra. 

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