Direct mass measurements establish that the 35.8 keV isomer in 129Sn acts as an astromer during neutron capture in the i-process and r-process.
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Exploration for Astromers near $^{132}$Sn with the Canadian Penning Trap
Direct mass measurements establish that the 35.8 keV isomer in 129Sn acts as an astromer during neutron capture in the i-process and r-process.