AIDA
GELINA
BRIKEN
nToF
CRIB
ISOLDE
CIRCE
nTOFCapture
DESPEC
DTAS
EDI_PSA
179Ta
CARME
StellarModelling
DCF
K40
BRIKEN
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Mon Mar 31 13:10:17 2025
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> AIDA plastic (veto) and Si de calibration > > For the calibration the Compton edge of the spectrum seen in the detectors was used. > There is a large uncertainty in that determination, since the spectra are not so clear in terms of shape. > > For the spectra V1A7C13_EFIR (Si de, top) the channel position is 12900 units > > For the spectra V1A7C14_EFIR (Si de, bottom) the channel position is 12950 units > > For the spectra V1A7C9_EFIR (AIDA plastic) the channel position is 10425 units > > These corresponds to the following calibration factors using 0.9 MeV as the Compton energy from Co source: > > V1A7C13_EFIR (Si de, top): 6.976744E-5 > V1A7C14_EFIR (Si de, bottom): 6.949807E-5 > V1A7C9_EFIR (AIDA plastic): 8.633094E-5
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