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tokens: We are thankful to the anonymous referee for providing constructive feedback that improved our manuscript. This research is supported by the National Science Foundation (USA) under grant No. PHY-1430152 (JINA Center for the Evolution of the Elements) and by the ERC Consolidator Grant (Hungary) funding scheme (project RADIOSTAR, G.A. n. 724560). K.B. acknowledges support from the NCN grants Sonata Bis 2 (DEC-2012/07/E/ST9/01360), OPUS (2015/19/B/ST9/01099), and OPUS (2015/19/B/ST9/03188). M.M., N.V., and R.S. are supported by the U.S. Department of Energy under contract No. DE-AC52-07NA27344 for the topical collaboration Fission In r -process Elements (FIRE). This work was also supported in part by the U.S. Department of Energy under grant No. DE-SC0013039 (R.S. and T.S.). A portion of this work was also carried out under the auspices of the National Nuclear Security Administration of the U.S. Department of Energy at Los Alamos National Laboratory under contract No. DE-AC52-06NA25396 (C.F., O.K., R.W., M.M.). This research used resources provided by the Los Alamos National Laboratory Institutional Computing Program (O.K., R.W.). Software: OMEGA (Côté et al. 2017b ), PRISM (Mumpower et al. 2017 ), StarTrack (Belczynski et al. 2002 , 2008 ), Los Alamos suite of statistical Hauser-Feshbach codes (Kawano 2016 ), NumPy (Van Der Walt et al. 2011 ), matplotlib ( https://matplotlib.org ).