The masses of 40 neutron-rich nuclides from Z = 51 to 64 were measured at an
average precision of δm/m=10−7 using the Canadian Penning Trap mass
spectrometer at Argonne National Laboratory. The measurements, of fission
fragments from a 252Cf spontaneous fission source in a helium gas catcher,
approach the predicted path of the astrophysical r process. Where overlap
exists, this data set is largely consistent with previous measurements from
Penning traps, storage rings, and reaction energetics, but large systematic
deviations are apparent in β-endpoint measurements. Differences in mass
excess from the 2003 Atomic Mass Evaluation of up to 400 keV are seen, as well
as systematic disagreement with various mass models.Comment: 15 pages, 16 figures. v2 updated, published in Physical Review