V. Palomar Schmidt Field centered on Selected Area 71 (1988)

Starlike objects with both blue and ultraviolet excess have been selected from a Palomar 1.2m Schmidt field centered on Kapteyn Selected Area 71. The method of selection is that used in the previous papers of this series, but modified to account for the differential reddening that occurs across the field. We list color classes, color sub-classes, positions, and magnitudes of the selected objects. https://ui.adsabs.harvard.edu/link_gateway/1988ApJS...66....1U/doi:10.1086/191242 https://ui.adsabs.harvard.edu/#abs/1988ApJS...66....1U/abstract

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Work Title V. Palomar Schmidt Field centered on Selected Area 71 (1988)
Access
Open Access
Creators
  1. Peter D. Usher
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
Acknowledgments
  1. A. Warnock III
  2. K.J. Mitchell
Related URLs
  1. https://ui.adsabs.harvard.edu/link_gateway/1988ApJS...66....1U/SIMBAD
  2. https://ui.adsabs.harvard.edu/link_gateway/1988ApJS...66....1U/NED
Deposited August 04, 2019

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Version 1
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    November 16, 2020 22:39 by Scholarsphere 4 Migration

  • Added 1988ApJS___66____1U.pdf

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  • Added Creator Peter D. Usher

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  • Published

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  • Updated

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Version 2
published

  • Created

    January 11, 2024 19:40 by pxu1

  • Updated

    January 11, 2024 19:40 by [unknown user]

  • Updated Work Title, Description, Publication Date Show Changes

    January 11, 2024 19:45 by pxu1

    Work Title
    • V. Palomar Schmidt Field centered on Selected Area 71 (1988)
    • Faint Blue Objects at High Galactic Latitude. V. Palomar Schmidt Field Centered on Selected Area 71”
    Description
    • Astrophysical Journal Supplement 66, 1–18, 1988. With K-L. Huang, K.J. Mitchell
    • Starlike objects with both blue and ultraviolet excess have been selected from a Palomar 1.2m Schmidt field centered on Kapteyn Selected Area 71. The method of selection is that used in the previous papers of this series, but modified to account for the differential reddening that occurs across the field. We list color classes, color sub-classes, positions, and magnitudes of the selected objects. https://ui.adsabs.harvard.edu/link_gateway/1988ApJS...66....1U/doi:10.1086/191242 https://ui.adsabs.harvard.edu/#abs/1988ApJS...66....1U/abstract
    Publication Date
    • 1988
  • Updated Acknowledgments Show Changes

    January 11, 2024 19:52 by pxu1

    Acknowledgments
    • A. Warnock III, K.J. Mitchell
  • Added Creator K.J. Mitchell

    January 11, 2024 19:52 by pxu1

  • Added Creator A. Warnock, III

    January 11, 2024 19:52 by pxu1

  • Updated Work Title, Description Show Changes

    January 11, 2024 19:54 by pxu1

    Work Title
    • Faint Blue Objects at High Galactic Latitude. V. Palomar Schmidt Field Centered on Selected Area 71”
    • Faint Blue Objects at High Galactic Latitude. V. Palomar Schmidt Field Centered on Selected Area 71
    Description
    • Astrophysical Journal Supplement 66, 1–18, 1988. With K-L. Huang, K.J. Mitchell
    • Astrophysical Journal Supplement 66, 1–18, 1988 (with K.J. Mitchell, A. Warnock, III).
    • Starlike objects with both blue and ultraviolet excess have been selected from a Palomar 1.2m Schmidt field centered on Kapteyn Selected Area 71. The method of selection is that used in the previous papers of this series, but modified to account for the differential reddening that occurs across the field. We list color classes, color sub-classes, positions, and magnitudes of the selected objects. https://ui.adsabs.harvard.edu/link_gateway/1988ApJS...66....1U/doi:10.1086/191242 https://ui.adsabs.harvard.edu/#abs/1988ApJS...66....1U/abstract
  • Published

    January 11, 2024 19:54 by pxu1

  • Updated

    April 04, 2024 10:22 by [unknown user]