Zobrazeno 1 - 10
of 31
pro vyhledávání: '"Fu-Chao Wu"'
Synthesis, crystal structures, and properties of three metal complexes with N-phenylanthranilic acid
Autor:
Tan, Yu-Hui, Xiong, Jian-Bo, Gao, Ji-Xing, Xu, Qing, Fu, Chao-Wu, Tang, Yun-Zhi, Yang, Shao-Ping, Wen, He-Rui
Publikováno v:
In Journal of Molecular Structure 15 April 2015 1086:49-55
Autor:
Tan, Yu-Hui, Yu, Yin-Mei, Xiong, Jian-Bo, Gao, Ji-Xing, Xu, Qing, Fu, Chao-wu, Tang, Yun-Zhi, Wen, He-Rui
Publikováno v:
In Polyhedron 9 March 2014 70:47-51
Autor:
Sen Yang, Fu-Chao Wu
Publikováno v:
Journal of Software. 22:2476-2487
Autor:
Fu-Chao Wu, Zhi-Heng Wang
Publikováno v:
Journal of Software. 19:803-816
Publikováno v:
Journal of Software. 19:2932-2942
Publikováno v:
Acta Automatica Sinica. 33:801-808
Central catadioptric cameras are widely used in virtual reality and robot navigation, and the camera calibration is a prerequisite for these applications. In this paper, we propose an easy calibration method for central catadioptric cameras with a 2D
Publikováno v:
Guang pu xue yu guang pu fen xi = Guang pu. 34(11)
At present, most sky-subtraction methods focus on the full spectrum, not the particular location, especially for the backgroud sky around [OIII] line which is very important to low redshift quasars. A new method to precisely subtract sky lines in loc
Publikováno v:
Chinese Astronomy and Astrophysics. 30:176-186
The physical parameters of stellar atmosphere, e.g. the effective temperature, surface gravity and chemical abundance, are the main factors for the differences in stellar spectra, and the automatic measurement of these parameters is an important cont
Publikováno v:
Guang pu xue yu guang pu fen xi = Guang pu. 30(6)
The authors present a new method called two class PCA for decomposing the mixed spectra, namely, for subtracting the host galaxy contamination from each SN spectrum. The authors improved the quality of reconstructed galaxy spectrum and computational
Publikováno v:
Guang pu xue yu guang pu fen xi = Guang pu. 29(12)
Supernova (SN) is one of the most intense astronomical phenomena among the known stellar activities, but compared with several billion astronomical objects which people have probed, the number of supernova the authors have observed is very small. The