Zobrazeno 1 - 10
of 696
pro vyhledávání: '"Li Chengdong"'
Autor:
Monjur, Mahathir, Liu, Jia, Xu, Jingye, Zhang, Yuntong, Wang, Xiaomeng, Li, Chengdong, Park, Hyejin, Wang, Wei, Shieh, Karl, Munir, Sirajum, Wang, Jing, Song, Lixin, Nirjon, Shahriar
This paper examines the application of WiFi signals for real-world monitoring of daily activities in home healthcare scenarios. While the state-of-the-art of WiFi-based activity recognition is promising in lab environments, challenges arise in real-w
Externí odkaz:
http://arxiv.org/abs/2402.09452
Autor:
Li, Chengdong, Yuan, Zhen, Monari, Giacomo, Martin, Nicolas F., Siebert, Arnaud, Famaey, Benoit, Chiba, Rimpei, Kordopatis, Georges, Ibata, Rodrigo A., Hill, Vanessa
Publikováno v:
A&A 690, A26 (2024)
The most metal-poor tail of the Milky Way ([Fe/H] $\leq$ $-$2.5) contains a population of stars with very prograde planar orbits, which is puzzling in both their origin and evolution. A possible scenario is that they are shepherded by the bar from th
Externí odkaz:
http://arxiv.org/abs/2311.15270
Autor:
Yuan, Zhen, Li, Chengdong, Martin, Nicolas F., Monari, Giacomo, Famaey, Benoit, Siebert, Arnaud, Ardern-Arentsen, Anke, Sestito, Federico, Thomas, Guillaume F., Hill, Vanessa, Ibata, Rodrigo A., Kordopatis, Georges, Starkenburg, Else, Viswanathan, Akshara
The most metal-poor stars (e.g. [Fe/H] $\leq-2.5$) are the ancient fossils from the early assembly epoch of our Galaxy, very likely before the formation of the thick disc. Recent studies have shown that a non-negligible fraction of them have prograde
Externí odkaz:
http://arxiv.org/abs/2311.08464
Autor:
Swisher, Earl
Publikováno v:
Eminent Chinese of the Qing Period, Rev ed., 2019.
Disc stars from the Gaia DR3 RVS catalogue are selected to explore the phase spiral as a function of position in the Galaxy. The data reveal a two-armed phase spiral pattern in the local $z-v_z$ plane inside the solar radius, which appears clearly wh
Externí odkaz:
http://arxiv.org/abs/2303.06393
Autor:
Li, Chengdong, Binney, James
We investigate the structure of our Galaxy's young stellar disc by fitting the distribution functions (DFs) of a new family to five-dimensional Gaia data for a sample of $47\,000$ OB stars. Tests of the fitting procedure show that the young disc's DF
Externí odkaz:
http://arxiv.org/abs/2205.01455
Autor:
Yan, Yan, Wu, Xuankun, Li, Chengdong, He, Yini, Zhang, Zhicheng, Li, Huihui, Li, Ang, Wang, Lei
Emotional recognition through exploring the electroencephalography (EEG) characteristics has been widely performed in recent studies. Nonlinear analysis and feature extraction methods for understanding the complex dynamical phenomena are associated w
Externí odkaz:
http://arxiv.org/abs/2203.06895
Publikováno v:
In Energy 15 October 2024 306
Publikováno v:
In Journal of Colloid And Interface Science September 2024 669:157-174
Publikováno v:
In Energy 1 August 2024 300