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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
Abstract
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.
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- Copyright © International Astronomical Union 2014