Colors of 2625 Quasars at 0 < z < 5 Measured in the Sloan Digital Sky Survey Photometric System

@article{Richards2000ColorsO2,
  title={Colors of 2625 Quasars at 0 < z < 5 Measured in the Sloan Digital Sky Survey Photometric System},
  author={Gordon T. Richards and Xiaohui Fan and Donald P. Schneider and Daniel E. vanden Berk and Michael A. Strauss and Donald G. York and John E. Anderson, Jr. and Scott F. Anderson and James T. Annis and Neta A. Bahcall and Mariangela Bernardi and John W. Briggs and Jonathan Brinkmann and Robert J. Brunner and Scott M. Burles and Larry N. Carey and Francisco J. Castander and Andrew J. Connolly and James H. Crocker and Istv{\'a}n Csabai and Mamoru Doi and Douglas P. Finkbeiner and Scott D. Friedman and Joshua A. Frieman and Masataka Fukugita and James E. Gunn and Robert B. Hindsley and Željko Ivezi{\'c} and Stephen Kent and Gillian R. Knapp and Donald Q. Lamb and R. French Leger and Daniel C. Long and Jon Loveday and Robert H. Lupton and Timothy A. Mckay and Avery Meiksin and Aronne Merrelli and Jeffrey A. Munn and Heidi Jo Newberg and M. G. Newcomb and Robert C. Nichol and Russell E. Owen and Jeffrey R. Pier and Adrian Pope and Michael Richmond and Constance M. Rockosi and David J. Schlegel and Walter A. Siegmund and Stephen A. Smee and Yehuda Snir and Chris Stoughton and Christopher W. Stubbs and Mark SubbaRao and Alexander S. Szalay and Gyula Pal Szokoly and Christy A. Tremonti and Alan K. Uomoto and Patrick Waddell and Brian Yanny and Wei Zheng},
  journal={The Astronomical Journal},
  year={2000},
  volume={121},
  pages={2308 - 2330}
}
We present an empirical investigation of the colors of quasars in the Sloan Digital Sky Survey (SDSS) photometric system. The sample studied includes 2625 quasars with SDSS photometry: 1759 quasars found during SDSS spectroscopic commissioning and SDSS follow-up observations on other telescopes, 50 matches to FIRST quasars, 573 matches to quasars from the NASA Extragalactic Database, and 243 quasars from two or more of these sources. The quasars are distributed in a 2.°5 wide stripe centered on… 

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