Fig. 6 from Characterization of M, L, and T Dwarfs in the Sloan Digital Sky Survey

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

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.

Provider: AAS Journals

Caption: Fig. 6.

SDSS spectra for objects M9 and later. The spectral types are ours, as given in Table 4, except for those for the L9 and T dwarfs, which are taken from previously published sources as described in the table notes. Note that we have not attempted to remove noise spikes such as those in the left panel of (e) near 6300 Å.

Other Images in This Article

Copyright and Terms & Conditions