Active Galactic Nuclei in the Sloan Digital Sky Survey. II. Emission-Line Luminosity Function

Lei Hao; Michael A. Strauss; Xiaohui Fan; Christy A. Tremonti; David J. Schlegel; Timothy M. Heckman; Guinevere Kauffmann; Michael R. Blanton; James E. Gunn; Patrick B. Hall; Željko Ivezić; Gillian R. Knapp; Julian H. Krolik; Robert H. Lupton; Gordon T. Richards; Donald P. Schneider; Iskra V. Strateva; Nadia L. Zakamska; J. Brinkmann; Gyula P. Szokoly

Journal ArticleOPEN ACCESS

Active Galactic Nuclei in the Sloan Digital Sky Survey. II. Emission-Line Luminosity Function

Hao L
Strauss M
Fan X
et al.

The Astronomical Journal (2005) 129(4) 1795-1808

DOI: 10.1086/428486

177Citations

46Readers

Abstract

The emission line luminosity function of active galactic nuclei (AGN) is measured from about 3000 AGN included in the main galaxy sample of the Sloan Digital Sky Survey within a redshift range of $0

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APA

Hao, L., Strauss, M. A., Fan, X., Tremonti, C. A., Schlegel, D. J., Heckman, T. M., … Szokoly, G. P. (2005). Active Galactic Nuclei in the Sloan Digital Sky Survey. II. Emission-Line Luminosity Function. The Astronomical Journal, 129(4), 1795–1808. https://doi.org/10.1086/428486

Active Galactic Nuclei in the Sloan Digital Sky Survey. II. Emission-Line Luminosity Function

Abstract

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