APA
Liu H. N., Obertelli A., Doornenbal P., Bertulani C. A., Hagen G., Holt J. D., Jansen G. R., Morris T. D., Schwenk A., Stroberg R., Achouri N., Baba H., Browne F., Calvet D., Château F., Chen S., Chiga N., Corsi A., Cortés M. L., Delbart A., Gheller J., Giganon A., Gillibert A., Hilaire C., Isobe T., Kobayashi T., Kubota Y., Lapoux V., Motobayashi T., Murray I., Otsu H., Panin V., Paul N., Rodriguez W., Sakurai H., Sasano M., Steppenbeck D., Stuhl L., Sun Y. L., Togano Y., Uesaka T., Wimmer K., Yoneda K., Aktas O., Aumann T., Chung L. X., Flavigny F., Franchoo S., Gašparić I., Gerst R., Gibelin J., Hahn K. I., Kim D., Koiwai T., Kondo Y., Koseoglou P., Lee J., Lehr C., Linh B. D., Lokotko T., MacCormick M., Moschner K., Nakamura T., Park S. Y., Rossi D., Sahin E., Sohler D., Söderström P., Takeuchi S., Törnqvist H., Vaquero V., Wagner V., Wang S., Werner V., Xu X., Yamada H., Yan D., Yang Z., Yasuda M. & Zanetti L. (20190313). How Robust is the N=34 Subshell Closure? First Spectroscopy of ^{52}Ar. : Physical review letters.
Chicago
Liu H N, Obertelli A, Doornenbal P, Bertulani C A, Hagen G, Holt J D, Jansen G R, Morris T D, Schwenk A, Stroberg R, Achouri N, Baba H, Browne F, Calvet D, Château F, Chen S, Chiga N, Corsi A, Cortés M L, Delbart A, Gheller J-M, Giganon A, Gillibert A, Hilaire C, Isobe T, Kobayashi T, Kubota Y, Lapoux V, Motobayashi T, Murray I, Otsu H, Panin V, Paul N, Rodriguez W, Sakurai H, Sasano M, Steppenbeck D, Stuhl L, Sun Y L, Togano Y, Uesaka T, Wimmer K, Yoneda K, Aktas O, Aumann T, Chung L X, Flavigny F, Franchoo S, Gašparić I, Gerst R-B, Gibelin J, Hahn K I, Kim D, Koiwai T, Kondo Y, Koseoglou P, Lee J, Lehr C, Linh B D, Lokotko T, MacCormick M, Moschner K, Nakamura T, Park S Y, Rossi D, Sahin E, Sohler D, Söderström P-A, Takeuchi S, Törnqvist H, Vaquero V, Wagner V, Wang S, Werner V, Xu X, Yamada H, Yan D, Yang Z, Yasuda M and Zanetti L. 20190313. How Robust is the N=34 Subshell Closure? First Spectroscopy of ^{52}Ar. : Physical review letters.
Harvard
Liu H. N., Obertelli A., Doornenbal P., Bertulani C. A., Hagen G., Holt J. D., Jansen G. R., Morris T. D., Schwenk A., Stroberg R., Achouri N., Baba H., Browne F., Calvet D., Château F., Chen S., Chiga N., Corsi A., Cortés M. L., Delbart A., Gheller J., Giganon A., Gillibert A., Hilaire C., Isobe T., Kobayashi T., Kubota Y., Lapoux V., Motobayashi T., Murray I., Otsu H., Panin V., Paul N., Rodriguez W., Sakurai H., Sasano M., Steppenbeck D., Stuhl L., Sun Y. L., Togano Y., Uesaka T., Wimmer K., Yoneda K., Aktas O., Aumann T., Chung L. X., Flavigny F., Franchoo S., Gašparić I., Gerst R., Gibelin J., Hahn K. I., Kim D., Koiwai T., Kondo Y., Koseoglou P., Lee J., Lehr C., Linh B. D., Lokotko T., MacCormick M., Moschner K., Nakamura T., Park S. Y., Rossi D., Sahin E., Sohler D., Söderström P., Takeuchi S., Törnqvist H., Vaquero V., Wagner V., Wang S., Werner V., Xu X., Yamada H., Yan D., Yang Z., Yasuda M. and Zanetti L. (20190313). How Robust is the N=34 Subshell Closure? First Spectroscopy of ^{52}Ar. : Physical review letters.
MLA
Liu H N, Obertelli A, Doornenbal P, Bertulani C A, Hagen G, Holt J D, Jansen G R, Morris T D, Schwenk A, Stroberg R, Achouri N, Baba H, Browne F, Calvet D, Château F, Chen S, Chiga N, Corsi A, Cortés M L, Delbart A, Gheller J-M, Giganon A, Gillibert A, Hilaire C, Isobe T, Kobayashi T, Kubota Y, Lapoux V, Motobayashi T, Murray I, Otsu H, Panin V, Paul N, Rodriguez W, Sakurai H, Sasano M, Steppenbeck D, Stuhl L, Sun Y L, Togano Y, Uesaka T, Wimmer K, Yoneda K, Aktas O, Aumann T, Chung L X, Flavigny F, Franchoo S, Gašparić I, Gerst R-B, Gibelin J, Hahn K I, Kim D, Koiwai T, Kondo Y, Koseoglou P, Lee J, Lehr C, Linh B D, Lokotko T, MacCormick M, Moschner K, Nakamura T, Park S Y, Rossi D, Sahin E, Sohler D, Söderström P-A, Takeuchi S, Törnqvist H, Vaquero V, Wagner V, Wang S, Werner V, Xu X, Yamada H, Yan D, Yang Z, Yasuda M and Zanetti L. How Robust is the N=34 Subshell Closure? First Spectroscopy of ^{52}Ar. : Physical review letters. 20190313.