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gssi-cryogroup:gagg-nd:first_month

A first look at a month of data from the GAGG

2024/2/27, AndreaM

We analyse roughly one month of data acquired with the GAGG underground, from 2024/1/15 to 2024/2/12. The dataset is 29 days long, the total number of acquired events is 38193181, which corresponds to a rate of ∼15 Hz.

We consider the discrimination parameter normamplitude η=Amplitude/Integral and we define the β/γ and α bands as follow:

  • β/γ : 0.03 < η <0.1
  • α : 0.01 < η < 0.03

The 2D plot in Figure 1 shows η vs Integral for the events.

Figure 1
Total 2D plot η vs Integral Zoom-in for Integral<82000

The large majority of the events (96%) is falling in the β/γ band. Beyond 208Tl peak there is a first population of order 900 events probably due to the overlap of the 2.6 MeV γ with another lower energy γ (583 keV, 511 keV,…). Then there is another population (only 8 events) around Integral = 150-200*103 which maybe is due to other γ overlaps or are we seeing some first γ from Gd-n capture?
NOTE: The range 150-200*103 in ADC counts corresponds to 5.8-7.7 MeV (as shown later in the note).

The β/γ band.

Figure 2

We recognize two clear peak in this spectrum: one around 40*103 which is due to the 1.5 MeV 40K decay and one at 70*103 from the 2.6 MeV 208Tl decay. Even if very preliminary, we can try a simple gaussian fit of these peaks.

Figure 3
40K fit 208Tl fit

Just to have a feeling, the following table reports the fit result and the first estimation of the energy resolution.

Peak Energy [MeV] Fit Mean [ADC] Fit Sigma [ADC] Energy Scale from fit [ADC/MeV] Energy Resolution (Sigma/Mean) [%]
40K 1.5 38100 1126 25400 2.9
208Tl 2.6 68060 1600 26180 2.3

The α band.

Figure 4

For the α events we have to consider a quenching effect. We can try to have a first estimation looking at some characteristic peaks of the α spectrum.

  • The narrow peak below 104 is due to the α-decay of 152Gd at 2.2 MeV. This represents the dominant feature in the α spectrum.
  • The peak slightly below 2*104 is probably a mixture of the 238U α-decays at 4.2 and 4.15 MeV. In the left tail some other α-decay is probably present, maybe the ∼4 MeV decays from 232Th.
  • The peak between 2-2.5*104 can be tentatively attributed to 234U decay at 4.78 and 4.72 MeV.
  • Finally with the delayed coincidence analysis we have identified the peak between 3.5-4*104 as due to 216Po α-decay at 6.8 MeV.

We can try again a simple gaussian fit of these 4 peaks.

Figure 5
152Gd [2.2 MeV] 238U [4.2 MeV]
234U [4.8 MeV] 216Po [6.8 MeV]

The following table summarises the results of the fit, with a tentive estimation of the quenching effect with respect to the energy scale derived from the β/γ band (∼26000 ADC/MeV).

α Peak Energy [MeV] Fit Mean [ADC] Fit Sigma [ADC] Energy Scale from fit [ADC/MeV] Quenching
152Gd 2.2 8452 347 3842 0.15
238U 4.2 19340 864 4605 0.18
234U 4.8 23150 818 4823 0.18
216Po 6.8 37430 1300 5504 0.21

Next steps

  1. Detailed study of α-α and α-γ delayed coincidences
  2. Conversion of ADC counts in number of PE
  3. Improve the discrimination parameter η
  4. AmBe calibration to see neutron captures
  5. Calibration with γ sources for detailed energy scale and resolution studies (?)
gssi-cryogroup/gagg-nd/first_month.txt · Last modified: by 127.0.0.1