Hu Zou - BATC home page
Hu Zou - BATC home page
Hu Zou - BATC home page
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– Based on the observations of the Chinese Small Telescope ARray (CSTAR) deployed at Antarctic<br />
Dome A in 2008, the i-band sky background brightness, transparency and the effect on the imaging<br />
by the Aurorae were analyzed. The paper about this work was published in AJ in 2010.<br />
– Using the panchromatic spectral energy distribution (SED) from ultraviolet, optical and infrared<br />
photometry, a nearby face-on spiral galaxy, NGC 628, was investigated to study its two-dimensional<br />
features. With the help of an evolutionary stellar population synthesis model (PEGASE), age,<br />
metallicity and reddening maps were obtained so that structures of the distinct bulge, disk and<br />
spiral arms and the formation and evolution history of the galaxy were understood. H II regions<br />
were specially treated due to their complex stellar populations in observations which were mixed<br />
with the galactic background populations. The paper was submitted to AJ.<br />
– With the commissioning data of the Guoshoujing Telescope (previously named LAMOST, the largest<br />
telescope built in China), we tried to derive the kinetic properties such as the velocity field and<br />
velocity dispersions and the features of stellar populations by STARLIGHT (a spectrum fitting code).<br />
Master Work<br />
– With the u, g, r, i and z photometric catalog over 40×20 deg 2 in the sixth data release of the Sloan<br />
Digital Sky Survey, the tidal tails of Palomar 5 were detected by the artificial neural networks<br />
technique. This method was proved to be a nice approach comparable with the optimal match<br />
filter method as usually adopted by most researchers in their studies of tidal tails.<br />
– For the accumulated data of 15 intermediate bands in the Beijing-Arizona-Taipei-Connecticut (<strong>BATC</strong>)<br />
survey during the last decades, an effective classifier was designed to separate stars and galaxies<br />
by employing the ANN method. This method was also applied to the classification of the morphological<br />
type of galaxies using tens of photometric parameters.<br />
Undergraduate Work<br />
– Designed a software package which can be invoked to simulate the fractals.<br />
Honors and Awards<br />
Excellent Tri-A Student Scholarship of Graduate University of Chinese Academy of Sciences, 2007<br />
Excellent Tri-A Student Scholarship of Central South University, 2003–2006<br />
Scholarship of Central South University, 2003–2006<br />
“Honorable Mention” in the Interdisciplinary Contest in Modeling of America (ICM), 2005<br />
National fellowship of China, 2004<br />
Prize in the China Undergraduate Mathematic Contest in Modeling (CUMCM), 2004<br />
Publications<br />
Journal Papers<br />
H. <strong>Zou</strong>, Z. Y. Wu, J. Ma, and X. Zhou. The Tidal Tails of Globular Cluster Palomar 5 Based on Neural<br />
Networks Method. Research in Astronomy and Astrophysics, 9(10):1131–1148, Oct. 2009.<br />
Zhang Wei, Li Cheng, Kauffmann, Guinevere, <strong>Zou</strong> <strong>Hu</strong>, Catinella Barbara, Shen shiyin, Guo Qi, and<br />
Chang Ruixiang. Estimating the HI gas fractions of galaxies in the local Universe. Monthly Notices<br />
of the Royal Astronomical Society, 397(3):1243–1253, Aug. 2009.<br />
<strong>Hu</strong> <strong>Zou</strong>, Xu Zhou, Zhaoji Jiang, M.C.B. Ashley, Xiangqun Cui, Longlong Feng, Xuefei Gong, Jingyao<br />
<strong>Hu</strong>, C. A. Kulesa, J.S. Lawrence, Genrong Liu, D.M. Luong-Van, Jun Ma, A. M. Moore, Weijia<br />
Qin, Zhaohui Shang, J.W.V. Storey, Bo Sun, T. Travouillon, C. K. Walker, Jiali Wang, Lifan Wang,<br />
Jianghua Wu, Zhenyu Wu, Lirong Xia, Jun Yan, Ji Yang, <strong>Hu</strong>igen Yang, Yongqiang Yao, Xiangyan<br />
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