II. Palomar Schmidt Field centered on Selected Area 29 (1982)

The paper contains the second part of a list of ultraviolet excess objects. The objects were selected from a Palomar 1.2 m Schmidt field centered on Kapteyn selected area 29. The population of objects belonging to color classes 1A, 1, and 1B should be comprised primarily of quasars and white dwarfs and should be statistically complete to about B = 18.5 mag. US943 (now DV UMa) is a Cataclysmic Variable star undergoing outbursts of 5 mag. It was discovered by Dianne Duncan (nee Mattson) when she was a Penn State undergraduate student. https://doi.org/10.1086/190767 http://adsabs.harvard.edu/abs/1982ApJS...48...51U https://doi:10.1126/science.1259063

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Work Title II. Palomar Schmidt Field centered on Selected Area 29 (1982)
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Open Access
Creators
  1. Peter D. Usher
Keyword
  1. US 943
  2. white dwarfs
  3. DV UMa
  4. quasars
  5. survey
License CC BY-NC-SA 4.0 (Attribution-NonCommercial-ShareAlike)
Work Type Research Paper
Acknowledgments
  1. D. Mattson
  2. A. Warnock III
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Deposited August 04, 2019

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Version 1
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  • Added 1982ApJS___48___51U.pdf
  • Added Creator Peter D. Usher
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Version 2
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  • Updated Work Title, Keyword, Description, and 1 more Show Changes
    Work Title
    • II. Palomar Schmidt Field centered on Selected Area 29 (1982)
    • Faint Blue Objects at High Galactic Latitude. II. Palomar Schmidt Field Centered on Selected Area 29
    Keyword
    • US 943, white dwarfs, DV UMa, quasars, survey
    • US 943, white dwarfs, DV UMa, quasars, survey, US 708
    Description
    • The paper contains the second part of a list of ultraviolet excess objects. The objects were selected from a Palomar 1.2 m Schmidt field centered on Kapteyn selected area 29. The population of objects belonging to color classes 1A, 1, and 1B should be comprised primarily of quasars and white dwarfs and should be statistically complete to about B = 18.5 mag. US943 (now DV UMa) is a Cataclysmic Variable star undergoing outbursts of 5 mag. It was discovered by Dianne Duncan (nee Mattson) when she was a Penn State undergraduate student. https://doi.org/10.1086/190767 http://adsabs.harvard.edu/abs/1982ApJS...48...51U https://doi:10.1126/science.1259063
    • Peter D. Usher, Dianne Mattson, Archibald Warnock III
    • https://ui.adsabs.harvard.edu/abs/1982ApJS...48...51U/abstract
    • The second part of a list of ultraviolet excess objects is given. The objects have been selected from a Palomar Schmidt field centered on Kapteyn selected area 29. The population of objects belonging to color classes 1A, 1, and 1B should be comprised primarily of quasars and white dwarfs and should be statistically complete to about B = 18.5 mag. One of the listed objects is a 5 mag optical variable; a journal of observations is given, derived from Harvard archival and contemporary Palomar Schmidt plates.US943 (now DV UMa) is a Cataclysmic Variable star undergoing outbursts of 5 mag. It was discovered by Dianne Duncan (nee Mattson) when she was a Penn State undergraduate student. http://adsabs.harvard.edu/abs/1982ApJS...48...51U https://doi:10.1126/science.1259063
    Publication Date
    • 1982
  • Updated Acknowledgments Show Changes
    Acknowledgments
    • D. Mattson, A. Warnock III
  • Added Creator Dianne Mattson
  • Added Creator Archibald Warnock III
  • Updated Description Show Changes
    Description
    • Peter D. Usher, Dianne Mattson, Archibald Warnock III
    • https://ui.adsabs.harvard.edu/abs/1982ApJS...48...51U/abstract
    • The second part of a list of ultraviolet excess objects is given. The objects have been selected from a Palomar Schmidt field centered on Kapteyn selected area 29. The population of objects belonging to color classes 1A, 1, and 1B should be comprised primarily of quasars and white dwarfs and should be statistically complete to about B = 18.5 mag. One of the listed objects is a 5 mag optical variable; a journal of observations is given, derived from Harvard archival and contemporary Palomar Schmidt plates.US943 (now DV UMa) is a Cataclysmic Variable star undergoing outbursts of 5 mag. It was discovered by Dianne Duncan (nee Mattson) when she was a Penn State undergraduate student. http://adsabs.harvard.edu/abs/1982ApJS...48...51U https://doi:10.1126/science.1259063
    • The second part of a list of ultraviolet excess objects is given. The objects have been selected from a Palomar Schmidt field centered on Kapteyn selected area 29. The population of objects belonging to color classes 1A, 1, and 1B should be comprised primarily of quasars and white dwarfs and should be statistically complete to about B = 18.5 mag. One of the listed objects is a 5 mag optical variable; a journal of observations is given, derived from Harvard archival and contemporary Palomar Schmidt plates. US 708 is a unique subdwarf O-star. US943 (now DV UMa) is a Cataclysmic Variable star undergoing outbursts of 5 mag. It was discovered by Dianne Duncan (nee Mattson) when she was a Penn State undergraduate student. http://adsabs.harvard.edu/abs/1982ApJS...48...51U https://doi:10.1126/science.1259063
  • Published
  • Updated

Version 3
published

  • Created
  • Updated Description, Publisher's Statement Show Changes
    Description
    • Peter D. Usher, Dianne Mattson, Archibald Warnock III
    • https://ui.adsabs.harvard.edu/abs/1982ApJS...48...51U/abstract
    • The second part of a list of ultraviolet excess objects is given. The objects have been selected from a Palomar Schmidt field centered on Kapteyn selected area 29. The population of objects belonging to color classes 1A, 1, and 1B should be comprised primarily of quasars and white dwarfs and should be statistically complete to about B = 18.5 mag. One of the listed objects is a 5 mag optical variable; a journal of observations is given, derived from Harvard archival and contemporary Palomar Schmidt plates. US 708 is a unique subdwarf O-star. US943 (now DV UMa) is a Cataclysmic Variable star undergoing outbursts of 5 mag. It was discovered by Dianne Duncan (nee Mattson) when she was a Penn State undergraduate student. http://adsabs.harvard.edu/abs/1982ApJS...48...51U https://doi:10.1126/science.1259063
    • The second part of a list of ultraviolet excess objects is given. The objects have been selected from a Palomar Schmidt field centered on Kapteyn selected area 29. The population of objects belonging to color classes 1A, 1, and 1B should be comprised primarily of quasars and white dwarfs and should be statistically complete to about B = 18.5 mag. One of the listed objects is a 5 mag optical variable; a journal of observations is given, derived from Harvard archival and contemporary Palomar Schmidt plates. US943 (now DV UMa) is a Cataclysmic Variable star undergoing outbursts of 5 mag. It was discovered by Dianne Duncan (nee Mattson) when she was a Penn State undergraduate student. http://adsabs.harvard.edu/abs/1982ApJS...48...51U https://doi:10.1126/science.1259063
    Publisher's Statement
    • US 708 is a unique subdwarf O-star. US 943 (now DV UMa) is a Cataclysmic Variable star undergoing outbursts of 5 mag discovered by Dianne Duncan (nee Mattson) when she was a Penn State undergraduate student.
  • Published
  • Updated

Version 4
published

  • Created
  • Updated Description Show Changes
    Description
    • Peter D. Usher, Dianne Mattson, Archibald Warnock III
    • https://ui.adsabs.harvard.edu/abs/1982ApJS...48...51U/abstract
    • The second part of a list of ultraviolet excess objects is given. The objects have been selected from a Palomar Schmidt field centered on Kapteyn selected area 29. The population of objects belonging to color classes 1A, 1, and 1B should be comprised primarily of quasars and white dwarfs and should be statistically complete to about B = 18.5 mag. One of the listed objects is a 5 mag optical variable; a journal of observations is given, derived from Harvard archival and contemporary Palomar Schmidt plates. US943 (now DV UMa) is a Cataclysmic Variable star undergoing outbursts of 5 mag. It was discovered by Dianne Duncan (nee Mattson) when she was a Penn State undergraduate student. http://adsabs.harvard.edu/abs/1982ApJS...48...51U https://doi:10.1126/science.1259063
  • Published
  • Updated