Figure 7 from ABUNDANCES, STELLAR PARAMETERS, AND SPECTRA FROM THE SDSS-III/APOGEE SURVEY

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

ABUNDANCES, STELLAR PARAMETERS, AND SPECTRA FROM THE SDSS-III/APOGEE SURVEY

Authors: Jon A. Holtzman, Matthew Shetrone , Jennifer A. Johnson, Carlos Allende Prieto, Friedrich Anders, Brett Andrews, Timothy C. Beers, Dmitry Bizyaev, Michael R. Blanton, Jo Bovy, Ricardo Carrera, S. Drew Chojnowski, Katia Cunha, Daniel J. Eisenstein, Diane Feuillet, Peter M. Frinchaboy, Jessica Galbraith-Frew, Ana E. García Pérez, D. A. García-Hernández, Sten Hasselquist, Michael R. Hayden, Fred R. Hearty, Inese Ivans, Steven R. Majewski, Sarah Martell, Szabolcs Meszaros, Demitri Muna, David Nidever, Duy Cuong Nguyen, Robert W. O'Connell, Kaike Pan, Marc Pinsonneault, Annie C. Robin, Ricardo P. Schiavon, Neville Shane, Jennifer Sobeck, Verne V. Smith, Nicholas Troup, David H. Weinberg, John C. Wilson, W. M. Wood-Vasey, Olga Zamora, and Gail Zasowski

2015 The Astronomical Journal 150 148.

Provider: AAS Journals

Caption: Figure 7.

Comparison with literature spectroscopic effective temperatures and surface gravities. Left panel is uncalibrated ASPCAP results; right is for calibrated results. Differences are ASPCAP minus reference values. Large circles are parameters from FTS spectra (Smith et al. 2013), filled triangles from optical spectra and analysis, and small points from globular cluster analysis of Mészáros et al. (2015).

Other Images in This Article

Copyright and Terms & Conditions