AIDA
GELINA
BRIKEN
nToF
CRIB
ISOLDE
CIRCE
nTOFCapture
DESPEC
DTAS
EDI_PSA
179Ta
CARME
StellarModelling
DCF
K40
StellarModelling
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Wed Mar 26 10:27:48 2025
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<p>This is the parameters of Ca42+n and Ca50+n acquired from differen models. They were chosen as they have Gaussian distributions which are consistent with TALYS calculations of MACS. Ca42+n has experimental values while Ca50+n does not.</p>
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