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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":"2018-09-09T15:09:04Z","abstract_excerpt":"Background: Beta-decay spectroscopy provides valuable nuclear physics input for thermonuclear reaction rates of astrophysical interest and stringent test for shell-model theories far from the stability line. Purpose: The available decay properties of proton drip-line nucleus $^{27}$S is insufficient to constrain the properties of the key resonance in $^{26}$Si$(p,\\gamma)^{27}$P reaction rate and probe the possible isospin asymmetry. The decay scheme of $^{27}$S is complicated and far from being understood, which has motivated but also presented challenges for our experiment. 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G. Wu, C. J. Lin, C. X. Yuan, D. Patel, D. S. Hou, D. W. Luo, D. X. Wang, F. F. Duan, F. P. Zhong, F. Yang, G. L. Zhang, G. M. Yu, G. Z. Shi, H. H. Sun, H. L. Zang, H. M. Jia, H. Q. Zhang, H. Y. Wu, J. B. Ma, J. G. Wang, J. J. He, J. Jos\\'e, J. Lee, J. S. Wang, L. J. Sun, L. Yang, L. Y. Hu, M. L. Liu, M. Pan, N. R. Ma, P. F. Liang, P. J. Li, P. Ma, P. 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":"2018-09-09T15:09:04Z","abstract_excerpt":"Background: Beta-decay spectroscopy provides valuable nuclear physics input for thermonuclear reaction rates of astrophysical interest and stringent test for shell-model theories far from the stability line. 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