no code implementations • 4 Nov 2014 • A. A. Miller, J. S. Bloom, J. W. Richards, Y. S. Lee, D. L. Starr, N. R. Butler, S. Tokarz, N. Smith, J. A. Eisner
In sum, the training set includes ~9000 spectra, for which stellar parameters are measured using the SEGUE Stellar Parameters Pipeline (SSPP).
Solar and Stellar Astrophysics Instrumentation and Methods for Astrophysics
