Stellar Population Studies with the SDSS. I. The Vertical Distribution of Stars in the Milky Way

@article{Chen2001StellarPS,
  title={Stellar Population Studies with the SDSS. I. The Vertical Distribution of Stars in the Milky Way},
  author={Bingqiu Chen and Chris Stoughton and J. Allyn Smith and Alan K. Uomoto and Jeffrey R. Pier and Brian Yanny and Željko Ivezi{\'c} and Donald G. York and J. Anderson and James T. Annis and Jonathan V. Brinkmann and Istv{\'a}n Csabai and Masataka Fukugita and Robert B. Hindsley and Robert H. Lupton and Jeffrey A. Munn},
  journal={The Astrophysical Journal},
  year={2001},
  volume={553},
  pages={184-197}
}
We present star count data from the Sloan Digital Sky Survey for 5.8 × 105 stars brighter than g' = 21 mag over 279 deg2 in two samples north and south of the Galactic plane. Using these high-latitude (49° < |b| < 64°) star counts we determine the Sun's distance from the Galactic midplane to be 27 ± 4 pc and the scale height of the old thin disk to be 330 ± 3 pc. Because of the photometric accuracy and large area sky coverage of these data, the color-magnitude diagram clearly reveals a… 
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