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Estimation of Galactic model parameters in high latitudes with the SDSS and SCUSS

Published online by Cambridge University Press:  06 January 2014

Cuihua Du
Affiliation:
School of Physics, University of Chinese Academy of Sciences, Beijing 100049, China email: ducuihua@ucas.ac.cn
Yunpeng Jia
Affiliation:
School of Physics, University of Chinese Academy of Sciences, Beijing 100049, China email: ducuihua@ucas.ac.cn
Xiyan Peng
Affiliation:
National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China
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Abstract

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Based on the South Galactic Cap U-band Sky Survey (SCUSS) and SDSS observation, we adopted the star-count method to analyze the stellar distribution in different directions of the Galaxy. We find that these model parameters may be variable with observed direction, which cannot simply be attributed to statistical errors.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2014 

References

Carollo, D., Beers, T. C., Lee, Y. S., 2008, Nature, 451, 216Google Scholar
Ivezić, Ž., et al. 2008, ApJ, 684, 287Google Scholar
Jurić, M., Ǐvezić, Z., et al. 2008, ApJ, 673, 864CrossRefGoogle Scholar
Siegel, M. H., Majewski, S. R., & Reid, I. N., 2002, ApJ, 578, 151CrossRefGoogle Scholar