Fig. 5 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. 5.

SDSS spectrum with highest signal‐to‐noise ratio at each spectral type. These spectra comprise a set of templates to be used in the SDSS pipeline processing for automatic spectral type identification in the future. Noise spikes near 5600 Å have not been removed.

Other Images in This Article

Copyright and Terms & Conditions