High-Redshift Quasars Found in Sloan Digital Sky Survey Commissioning Data. IV. Luminosity Function from the Fall Equatorial Stripe Sample

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X-Ray Emission from Radio-Quiet Quasars in the Sloan Digital Sky Survey Early Data Release: The αox Dependence upon Ultraviolet Luminosity (2002, methodology): “The z > 4 Sample: Chandra and XMM-Newton Observations All but one of the z > 4 SDSS quasars in the X-ray sample have been observed by Chandra, the only exception being the z = 5.74 quasar (Fan et al. 2000b) detected by XMM-Newton (Brandt et al. 2001).”
Seventy-One New L and T Dwarfs from the Sloan Digital Sky Survey (2006, background): “…(Fan et al. 1999, 2000b, 2001a, 2001b, 2003, 2004; Zheng et al. 2000) to the faintest and nearest stars and brown dwarfs (Kirkpatrick et al. 1999, 2000; Burgasser et al. 1999, 2002b; Fan et al. 2000a; Leggett et al. 2000; Geballe et al. 2002, hereafter G02; Knapp et al. 2004, hereafter K04).”
THE FINAL SDSS HIGH-REDSHIFT QUASAR SAMPLE OF 52 QUASARS AT z > 5.7 (2016, background): “Note that seven main-survey quasars are also located in overlap regions, and they are marked as “M+O.” Most of the 52 quasars were found by Fan et al. (2000, 2001a, 2001b, 2003, 2004, 2006a, 2006b) and Jiang et al. (2008,2009,2015, and this paper).”