Faint Blue Objects at High Galactic Latitude. IV. Palomar Schmidt Fields Centered on Selected Areas 55 and 94

K-L. Huang, P.D. Usher https://ui.adsabs.harvard.edu/link_gateway/1984ApJS...56..393H/doi:10.1086/190990, https://ui.adsabs.harvard.edu/#abs/1984ApJS...56..393H/abstract

Color classes, sub-classes, and approximate positions and magnitudes are ascertained for UV-excess objects that have been selected from Palomar Schmidt fields centered on Selected Areas 55 and 94. The method of selection uses the relative colors of the halo subdwarfs. The three-color imagery of the Tonantzintla technique also permits a mnemonic sub-classification.

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Work Title Faint Blue Objects at High Galactic Latitude. IV. Palomar Schmidt Fields Centered on Selected Areas 55 and 94
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Open Access
Creators
  1. Peter D. Usher
  2. Ke-Liang Huang
Keyword
  1. white dwarfs
  2. quasars
  3. survey
  4. blue stars
License CC BY-NC-SA 4.0 (Attribution-NonCommercial-ShareAlike)
Work Type Research Paper
Publication Date 1984
Deposited August 04, 2019

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Version 1
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Version 2
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  • Updated Work Title, Description Show Changes
    Work Title
    • IV. Palomar Schmidt Field centered on Selected Areas 55 and 94 (1984)
    • Faint Blue Objects at High Galactic Latitude. IV. Palomar Schmidt Fields Centered on Selected Areas 55 and 94
    Description
    • Color classes, sub-classes, and approximate positions and magnitudes are ascertained for UV-excess objects that have been selected from Palomar Schmidt fields centered on Selected Areas 55 and 94. The method of selection uses the relative colors of the halo subdwarfs. The three-color imagery of the Tonantzintla technique also permits a mnemonic sub-classification. https://ui.adsabs.harvard.edu/link_gateway/1984ApJS...56..393H/doi:10.1086/190990, https://ui.adsabs.harvard.edu/#abs/1984ApJS...56..393H/abstract
    • K-L. Huang, P.D. Usher
    • https://ui.adsabs.harvard.edu/link_gateway/1984ApJS...56..393H/doi:10.1086/190990, https://ui.adsabs.harvard.edu/#abs/1984ApJS...56..393H/abstract
    • Color classes, sub-classes, and approximate positions and magnitudes are ascertained for UV-excess objects that have been selected from Palomar Schmidt fields centered on Selected Areas 55 and 94. The method of selection uses the relative colors of the halo subdwarfs. The three-color imagery of the Tonantzintla technique also permits a mnemonic sub-classification.
  • Updated Acknowledgments Show Changes
    Acknowledgments
    • K-L. Huang
  • Updated Related URLs, Publication Date Show Changes
    Related URLs
    • https://ui.adsabs.harvard.edu/link_gateway/1984ApJS...56..393H/SIMBAD, https://ui.adsabs.harvard.edu/link_gateway/1984ApJS...56..393H/NED
    Publication Date
    • 1984
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Version 3
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  • Created
  • Added Creator Huang
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Version 4
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  • Renamed Creator Ke-Liang Huang Show Changes
    • Huang
    • Ke-Liang Huang
  • Published
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