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Wang, P. W. Wen, Q. Hu, Q. Q. Zhao, Q. W. Zhou, R. F. Chen, R. Li, S. Q. Hou, S. Y. Jin, W. H. Ma, W. Q. Yang, X. Wang, X. X. Xu, X. Y. Wang, Y. C. Yu, Y. F. Wang, Y. H. Lam, Y. Jiang, Y. Liu, Y. M. Zhao, Y. Y. Yang, Z. Bai, Z. G. Hu, Z. H. Gao, Z. H. Li","submitted_at":"2019-09-25T10:02:55Z","abstract_excerpt":"$\\beta$ decay of $^{26}$P was used to populate the astrophysically important $E_x=$5929.4(8) keV $J^{\\pi}=3{^+}$ state of $^{26}$Si. Both $\\beta$-delayed proton at 418(8) keV and gamma ray at 1742(2) keV emitted from this state were measured simultaneously for the first time with corresponding absolute intensities of 11.1(12)\\% and 0.59(44)\\%, respectively. Besides, shell model calculations with weakly bound effects were performed to investigate the decay properties of other resonant states and a spin-parity of $4^+$ rather than $0^+$ was favored for the $E_x=$5945.9(40) keV state. 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