{"paper":{"title":"Insight-HXMT observations of the New Black Hole Candidate MAXI J1535-571: timing analysis","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A.K.H. Kong, A. M. Zhang, B. B. Wu, B. Li, B. Lu, B. Meng, C. C. Guo, C. Gungor, C. K. Li, C. L. Zhang, C. L. Zou (The Insight-HXMT Collaboration), C. M. Zhang, C. Z. Liu, D. W. Han, F. G. Xie, F. J. Lu, F. Zhang, G. B. Zhang, G. Chen, G. C. Xiao, G. F. Wang, G. H. Gao, G. Li, G Ou, G. Q. Liu, H. Gao, H.-K. Chang, H. M. Zhang, H. S. Zhao, H. W. Liu, H. Xu, H. Y. Wang, J. F. Ji, J. F. Zhou, J. Guan, J. Huo, J. Jin, J. K. Deng, J. L. Qu, J. L. Zhao, J. Wang, J. W. Yang, J. Y. Liao, J. Y. Nie, J. Zhang, L. Chen, L. H. Jiang, L. L. Yan, L. M. Song, L. Sun, L. Tao, M. Gao, M. S. Li, M. Wu, M. X. Fu, M. Y. Ge, N. Sai, Q. C. Bu, Q. Zhang, R. C. Shang, S. J. Zheng, S. L. Xiong, S. M. Jia, S. N. Zhang, S. S. Weng, S.Yang, S. Zhang, S. Z. Liu, T. Luo, T. P. Li, T. X. Chen, T. Zhang, W. C. Jiang, W. Cui, W. C. Zhang, W. f. Yu, W. Hu, W. Li, W. S. Wang, W. Tao, W. W. Cui, W. Zhang, W. Z. Zhang, X. B. Li, X. F. Li, X. F. Lu, X. F. Zhao, X. H. Liang, X. Hou, X. J. Liu, X. L. Cao, X. Li, X. Ma, X. Y. Wen, Y. B. Chen, Y. Chen, Y. D. Gu, Y. F. Zhang, Y. G. Li, Y. Huang, Y. J. Jin, Y. J. Yang, Y. J. Zhang, Y. Liu, Y. L. Tuo, Y. Nang, Y. N. Liu, Y. P. Chen, Y. P. Xu, Y. S. Wang, Y. Tan, Y. W. Dong, Y. X. Zhu, Y. Y. Du, Y. Zhang, Y. Zhu, Z. Chang, Z. J. Li, Z. L. Zhang, Z. W. Li, Z. Zhang","submitted_at":"2018-08-16T00:53:41Z","abstract_excerpt":"We present the X-ray timing results of the new black hole candidate (BHC) MAXI J1535-571 during its 2017 outburst from Hard X-ray Modulation Telescope (\\emph{Insight}-HXMT) observations taken from 2017 September 6 to 23. Following the definitions given by \\citet{Belloni2010}, we find that the source exhibits state transitions from Low/Hard state (LHS) to Hard Intermediate state (HIMS) and eventually to Soft Intermediate state (SIMS). Quasi-periodic oscillations (QPOs) are found in the intermediate states, which suggest different types of QPOs. With the large effective area of \\emph{Insight}-HX"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1808.05318","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}