The structure of the galactic halo: SDSS versus SuperCOSMOS

@article{Xu2007TheSO,
  title={The structure of the galactic halo: SDSS versus SuperCOSMOS},
  author={Y. Xu and L. Deng and J. Hu},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={2007},
  volume={379},
  pages={1373-1389}
}
  • Y. Xu, L. Deng, J. Hu
  • Published 2007
  • Physics
  • Monthly Notices of the Royal Astronomical Society
  • The halo structure at high Galactic latitudes near both the north and south poles is studied using Sloan Digital Sky Survey (SDSS) and SuperCOSMOS data. For the south cap halo, the archive of the SuperCOSMOS photographic photometry sky survey is used. The coincident source rate between SuperCOSMOS data in B J band from 16.5 to 20.5 mag and SDSS data is about 92 per cent, in a common sky area in the south. While that in the R F band is about 85 per cent from 16.5 to 19.5 mag. Transformed to the… CONTINUE READING
    10 Citations
    The Dark Energy Survey: Prospects for resolved stellar populations
    • 20
    • PDF
    Mapping the Asymmetric Thick Disk: The Hercules Thick-Disk Cloud
    • 11
    • PDF
    The stellar halo of the Galaxy
    • 150
    • PDF
    Mapping the Milky Way with LAMOST I: method and overview
    • 12
    • PDF
    The LEGUE input catalog for dark night observing in the LAMOST pilot survey
    • 16
    • PDF

    References

    SHOWING 1-10 OF 13 REFERENCES
    The asymmetric structure of the Galactic halo
    • 17
    • PDF
    Stellar Population Studies with the SDSS. I. The Vertical Distribution of Stars in the Milky Way
    • 264
    The structure of the Galactic halo.
    • 44
    The SuperCOSMOS Sky Survey – I. Introduction and description
    • 461
    • Highly Influential
    • PDF
    Models for the Galaxy and the Predicted Star Counts
    • 642