AIDA
GELINA
BRIKEN
nToF
CRIB
ISOLDE
CIRCE
nTOFCapture
DESPEC
DTAS
EDI_PSA
179Ta
CARME
StellarModelling
DCF
K40
BRIKEN
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Fri Mar 31 03:54:26 2017
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There is a strong background line at ~1293 keV. According to the attached document this could come from the neutron activation of 115In to 116In (14s halflife) of Indium seals.
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natural-gammas.pdf
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