Zobrazeno 1 - 10
of 81
pro vyhledávání: '"Xu-Zhi Li"'
Publikováno v:
The Astrophysical Journal, Vol 967, Iss 2, p 94 (2024)
In this paper, we use two methods, an algorithm of the density-based spatial clustering of applications with noise combined with the Gaussian mixture model, and the maximum likelihood method, to study two open clusters: IC 2488 and IC 2714 with Gaia
Externí odkaz:
https://doaj.org/article/b902b17e5c7847f6ac1fe35c7cd22d12
Publikováno v:
The Astrophysical Journal Supplement Series, Vol 271, Iss 1, p 32 (2024)
Starting from more than 11,200 short-period (less than 0.5 days) EW-type eclipsing binary candidates with the All-Sky Automated Survey for Supernovae V -band light curves, we use the Markov Chain Monte Carlo algorithm and neural networks to obtain th
Externí odkaz:
https://doaj.org/article/db0371c2ae7b46bfa0bea64d177a95cf
Autor:
Wang, Wen-Yu a, Song, Ya-Mei a, Zhang, Jia-Nuo a, Zhao, Ming-Yue a, Pei, Wen-Han b, Zhang, Hui a, Yin, Hai-Bo a, Xu, Zhi-Li a, Xin, Gui-Zhong c, Xie, Ming a, Kang, Ting-Guo a, Chen, Yue-Hua a, ⁎, Song, Hui-Peng a, ⁎
Publikováno v:
In Journal of Chromatography B 1 October 2024 1246
Akademický článek
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Akademický článek
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Publikováno v:
In International Immunopharmacology July 2019 72:275-283
Variable stars play a key role in understanding the Milky Way and the universe. The era of astronomical big data presents new challenges for quick identification of interesting and important variable stars. Accurately estimating the periods is the mo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0fc4601ad5e02b9819320ac90d2ae07c
http://arxiv.org/abs/2212.10037
http://arxiv.org/abs/2212.10037
Publikováno v:
Publications of the Astronomical Society of Japan. 73:1486-1496
An open cluster is an ideal region to study the evolution of stars. In this work, we use Gaia Early Data Release 3 (Gaia EDR3) to derive the fundamental parameters of 30 faint open clusters listed in the catalogue given by Cantat-Gaudin et al. (2018,
Publikováno v:
IEEE Transactions on Reliability. 70:1071-1083
Model checking is a powerful technique for verifying the correctness of systems with respect to the requirements. While some errors happen in the property, the model itself, or the environment, we think that satisfaction of the property is meaningles
Publikováno v:
Publications of the Astronomical Society of Japan. 73:786-794
Contact binary stars are important research objects in astrophysics. The calculation speed of deriving the parameters of contact binaries with the Wilson–Devinney program and the Phoebe with Markov chain Monte Carlo (MCMC) program is relatively slo