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Reiser, J. T.*; Neeway, J. J.*; Cooley, S. K.*; Parruzot, B.*; Heredia-Langner, A.*; Gin, S.*; Thomas, M.*; Smith, N. J.*; Icenhower, J. P.*; Stone-Weiss, N.*; et al.
International Journal of Applied Glass Science, 16(4), p.e16707_1 - e16707_16, 2025/10
Times Cited Count：0 Percentile：0.00(Materials Science, Ceramics)Dimitriou, P.*; Basunia, S*; Bernstein, L.*; Chen, J.*; Elekes, Z.*; Huang, X.*; Hurst, A.*; Iimura, Hideki; Jain, A. K.*; Kelley, J.*; et al.
EPJ Web of Conferences, 239, p.15004_1 - 15004_4, 2020/09
Times Cited Count：0 Percentile：0.00(Nuclear Science & Technology)The Evaluated Nuclear Structure Data File (ENSDF) includes the most extensive and comprehensive set of nuclear structure and decay data evaluations performed by the international network of Nuclear Structure and Decay Data evaluators (NSDD) under the auspices of the IAEA. In this report we describe some of the recent NSDD activities and provide future perspectives.
-decay branching ratio of 
PtCubiss, J. G.*; Harding, R. D.*; Andreyev, A. N.; Althubiti, N.*; Andel, B.*; Antalic, S.*; Barzakh, A. E.*; Cocolios, T. E.*; Day Goodacre, T.*; Farooq-Smith, G. J.*; et al.
Physical Review C, 101(1), p.014314_1 - 014314_4, 2020/01
Times Cited Count：5 Percentile：41.84(Physics, Nuclear)The -decay branching ratio of 0.52(5)% from the ground state of Pt to the ground state of the daughter nucleus 
Os has been determined more precisely than before. The Pt was produced as the 
-decay granddaughter of Hg which was produced and separated with the CERN-ISOLDE facility. The reduced -decay width calculated with the present result has provided a new picture of the systematics for the -decay width of neutron-deficient Pt isotopes.
Hg, 
Hg, 
Hg and 
HgWrzosek-Lipska, K.*; Rezynkina, K.*; Bree, N.*; Zieli
ska, M.*; Gaffney, L. P.*; Petts, A.*; Andreyev, A. N.; Bastin, B.*; Bender, M.*; Blazhev, A.*; et al.
European Physical Journal A, 55(8), p.130_1 - 130_23, 2019/08
Times Cited Count：18 Percentile：80.96(Physics, Nuclear)
Sn and spin-orbit splitting in neutron-rich nucleiOrlandi, R.; Pain, S. D.*; Ahn, S.*; Jungclaus, A.*; Schmitt, K. T.*; Bardayan, D. W.*; Catford, W. N.*; Chapman, R.*; Chipps, K. A.*; Cizewski, J. A.*; et al.
Physics Letters B, 785, p.615 - 620, 2018/10
Times Cited Count：10 Percentile：58.26(Astronomy & Astrophysics)
-spectroscopy at an intense cold neutron beam facilityJentschel, M.*; Blanc, A.*; de France, G.*; K
ster, U.*; Leoni, S.*; Mutti, P.*; Simpson, G.*; Soldner, T.*; Ur, C.*; Urban, W.*; et al.
Journal of Instrumentation (Internet), 12(11), p.P11003_1 - P11003_33, 2017/11
Times Cited Count：45 Percentile：84.88(Instruments & Instrumentation)-delayed fission of 
AmWilson, G. L.*; Takeyama, Mirei*; Andreyev, A. N.; Andel, B.*; Antalic, S.*; Catford, W. N.*; Ghys, L.*; Haba, Hiromitsu*; He
berger, F. P.*; Huang, M.*; et al.
Physical Review C, 96(4), p.044315_1 - 044315_7, 2017/10
Times Cited Count：9 Percentile：54.53(Physics, Nuclear)Gaffney, L. P.*; Robinson, A. P.*; Jenkins, D. G.*; Andreyev, A. N.; Bender, M.*; Blazhev, A.*; Bree, N.*; Bruyneel, B.*; Butler, P.*; Cocolios, T. E.*; et al.
Physical Review C, 91(6), p.064313_1 - 064313_11, 2015/06
Times Cited Count：11 Percentile：57.28(Physics, Nuclear)
Ni; Spectroscopy of the N=49 isotope 
ZnOrlandi, R.; M
cher, D.*; Raabe, R.*; Jungclaus, A.*; Pain, S. D.*; Bildstein, V.*; Chapman, R.*; De Angelis, G.*; Johansen, J. G.*; Van Duppen, P.*; et al.
Physics Letters B, 740, p.298 - 302, 2015/01
Times Cited Count：29 Percentile：83.94(Astronomy & Astrophysics)
value in 
KrR
gis, J.-M.*; Jolie, J.*; Saed-Samii, N.*; Warr, N.*; Pfeiffer, M.*; Blanc, A.*; Jentschel, M.*; Kster, U.*; Mutti, P.*; Soldner, T.*; et al.
Physical Review C, 90(6), p.067301_1 - 067301_4, 2014/12
Times Cited Count：24 Percentile：78.85(Physics, Nuclear)Chadwick, M. B.*; Herman, M.*; Oblo
insk
, P.*; Dunn, M. E.*; Danon, Y.*; Kahler, A. C.*; Smith, D. L.*; Pritychenko, B.*; Arbanas, G.*; Arcilla, R.*; et al.
Nuclear Data Sheets, 112(12), p.2887 - 2996, 2011/12
Times Cited Count：2336 Percentile：99.99(Physics, Nuclear)The ENDF/B-VII.1 library is our latest recommended evaluated nuclear data file for use in nuclear science and technology applications, and incorporates advances made in the five years since the release of ENDF/B-VII.0. These advances focus on neutron cross sections, covariances, fission product yields and decay data, and represent work by the US Cross Section Evaluation Working Group (CSEWG) in nuclear data evaluation that utilizes developments in nuclear theory, modeling, simulation, and experiment. It features extension of covered nuclei, covariance data for 190 nuclei, R-matrix analyses of neutron reactions on light nuclei, updates for some medium-heavy and actinoid nuclei, etc. Criticality benchmark tests with a transport simulation code MCNP shows improved performances.
Smith, M. S.*; Lingerfelt, E. J.*; Scott, J. P.*; Nesaraja, C. D.*; Chae, K.*; Koura, Hiroyuki; Roberts, L. F.*; Hix, W. R.*; Bardayan, D. W.*; Blackmon, J. C.*
Proceedings of Science (Internet), 28, p.180_1 - 180_5, 2010/12
A Computational Infrastructure for Nuclear Astrophysics has been developed to streamline the inclusion of the latest nuclear physics data in astrophysics simulations. The infrastructure consists of a platform-indepedent suite of codes that are freely vailable online at nucastrodata.org. The newest features of, and future plans for, this software suite are give in.
MgDaecon, A. N.*; Smith, J. F.*; Freeman, S. J.*; Janssens, R. V. F.*; Carpenter, M. P.*; Hadinia, B.*; Hoffman, C. R.*; Kay, B. P.*; Lauritsen, T.*; Lister, C. J.*; et al.
Physical Review C, 82(3), p.034305_1 - 034305_7, 2010/09
Times Cited Count：24 Percentile：76.71(Physics, Nuclear)no abstracts in English
Smith, M. S.*; Lingerfelt, E. J.*; Scott, J. P.*; Nesaraja, C. D.*; Hix, W. R.*; Chae, K.*; Koura, Hiroyuki; Meyer, R. A.*; Bardayan, D. W.*; Blackmon, J. C.*; et al.
AIP Conference Proceedings 847, p.470 - 472, 2006/07
no abstracts in English
Anghel, A.*; Takahashi, Yoshikazu; Smith, S.*; Pourrahimi, S.*; Zhelamskij, M.*; Blau, B.*; Fuchs, A.*; Heer, B.*; Hamada, Kazuya; Fujisaki, H.*; et al.
Fusion Technology 1996, p.185 - 190, 1996/00
no abstracts in English
Zn and the structure of NiOrlandi, R.; Mcher, D.*; Raabe, R.*; Jungclaus, A.*; Pain, S. D.*; Bildstein, V.*; Chapman, R.*; De Angelis, G.*; Johansen, J. G.*; Van Duppen, P.*; et al.
no journal, ,
Smith, M. S.*; Kondev, F.*; Koura, Hiroyuki; Lingerfelt, E. J.*; Buckner, K.*; Nesaraja, C. D.*
no journal, ,
no abstracts in English
Smith, M. S.*; Lingerfelt, E. J.*; Buckner, K.*; Nesaraja, C. D.*; Koura, Hiroyuki; Kondev, F.*
no journal, ,
The masses of exotic nuclei near the limits of stability play an important role in a wide variety of studies, such as simulations of r-process nucleosynthesis occurring in supernovae, determination of reaction cross sections of halo nuclei, and global models of the structure of nuclei. To handle this amount of mass information, we have built an online, dedicated suite of codes. Our system, freely available at nuclearmasses.org, is a platform-independent client-server application. With our system, researchers can upload their own mass datasets, store them, share them with colleagues, and quickly and easily visualize them in customizable one- and two-dimensional plots. Mass dataset analysis tools are also available, enabling the average RMS differences between a reference dataset and numerous other sets to be determined. We have recently added the capability to visualize the two-neutron separation energy surface. More analysis tools will be developed for our suite.
Smith, M. S.*; Lingerfelt, E. J.*; Nesaraja, C. D.*; Koura, Hiroyuki; Kondev, F. G.*
no journal, ,
The masses of nuclei play an important role in a wide variety of studies, such as simulations of r-process nucleosynthesis occurring in supernovae, global models of the structure of nuclei, and statistical model calculations of reaction cross sections. More, mass measurements are being made than ever before. To handle the substantial amount of new mass information, we have built an online suite of codes that enables researchers to quickly and efficiently visualize and analyze nuclear mass datasets. Our system is a platform-independent client-server application that accommodates the latest mass measurements and theoretical mass models. We have provided a first set of mass dataset analysis tools which can switch from 2d plots of masses to plots of separation energies. We have recently added the capability to visualize the two-neutron separation energy surface. The website hosting our code suite also provides an easy mechanism to inform the community of nuclear masses.
Sn studied via the 
Sn(d,t)Sn reactionOrlandi, R.; Pain, S. D.*; Bardayan, D. W.*; Gross, C. J.*; Smith, M. S.*; Jungclaus, A.*; Ahn, S.*; Jones, K. L.*; Pittman, S. T.*; Schmitt, K. T.*; et al.
no journal, ,
