The Ultraviolet-To-Mid-Infrared Spectral Energy Distribution of Weak Emission Line Quasars

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This article presents Spitzer Space Telescope photometry of 18 Sloan Digital Sky Survey quasars which have weak or undetectable high-ionization emission lines in their rest-frame ultraviolet spectra.

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10 p.

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Lane, Ryan A.; Shemmer, Ohad; Diamond-Stanic, Aleksandar M.; Fan, Xiaohui; Anderson, Scott F.; Brandt, William Nielsen et al. September 23, 2011.

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This article presents Spitzer Space Telescope photometry of 18 Sloan Digital Sky Survey quasars which have weak or undetectable high-ionization emission lines in their rest-frame ultraviolet spectra.

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10 p.

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  • The Astrophysical Journal, 2011. Washington, DC: The American Astronomical Society.

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  • Publication Title: The Astrophysical Journal
  • Volume: 743
  • Page Start: 1
  • Page End: 10
  • Peer Reviewed: Yes

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  • September 23, 2011

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  • June 30, 2016, 3:10 p.m.

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  • Aug. 19, 2016, 3:32 p.m.

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Lane, Ryan A.; Shemmer, Ohad; Diamond-Stanic, Aleksandar M.; Fan, Xiaohui; Anderson, Scott F.; Brandt, William Nielsen et al. The Ultraviolet-To-Mid-Infrared Spectral Energy Distribution of Weak Emission Line Quasars, article, September 23, 2011; Washington, DC. (digital.library.unt.edu/ark:/67531/metadc849985/: accessed September 22, 2018), University of North Texas Libraries, Digital Library, digital.library.unt.edu; crediting UNT College of Arts and Sciences.