Figure 12 from ABUNDANCES, STELLAR PARAMETERS, AND SPECTRA FROM THE SDSS-III/APOGEE SURVEY

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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 12.

Effective temperature—surface gravity—metallicity distributions for uncalibrated full APOGEE sample (top) and for calibrated giant sample (bottom). Isochrones from Bressan et al. (2012) for a 4 Gyr population, with metallicities [M/H] = −1.8, −1.5, −1.0, −0.5, 0., 0.3 are overlaid.

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