Fig. 12 from Characterization of M, L, and T Dwarfs in the Sloan Digital Sky Survey

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Characterization of M, L, and T Dwarfs in the Sloan Digital Sky Survey

Authors: Suzanne L. Hawley, Kevin R. Covey, Gillian R. Knapp, David A. Golimowski, Xiaohui Fan, Scott F. Anderson, James E. Gunn, Hugh C. Harris, Željko Ivezić, Gary M. Long, Robert H. Lupton, Peregrine M. McGehee, Vijay Narayanan, Eric Peng, David Schlegel, Donald P. Schneider, Emily Y. Spahn, Michael A. Strauss, Paula Szkody, Zlatan Tsvetanov, Lucianne M. Walkowicz, J. Brinkmann, Michael Harvanek, Gregory S. Hennessy, S. J. Kleinman, Jurek Krzesinski, Dan Long, Eric H. Neilsen, Peter R. Newman, Atsuko Nitta, Stephanie A. Snedden, and Donald G. York

Hawley et al. 2002 The Astronomical Journal 123 3409.

Caption: Fig. 12.

Photometric parallax relations for colors formed from the r*, i*, z*, and 2MASS J magnitudes. Symbols are the same as in Fig. 11.