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Accurate Atmospheric Parameters at Moderate Resolution Using Spectral Indices: Preliminary Application to the MARVELS Survey

  • Authors: Luan Ghezzi, Letícia Dutra-Ferreira, Diego Lorenzo-Oliveira, Gustavo F. Porto de Mello, Basílio X. Santiago, Nathan De Lee, Brian L. Lee, Luiz N. da Costa, Marcio A. G. Maia, Ricardo L. C. Ogando, John P. Wisniewski, Jonay I. González Hernández, Keivan G. Stassun, Scott W. Fleming, Donald P. Schneider, Suvrath Mahadevan, Phillip Cargile, Jian Ge, Joshua Pepper, Ji Wang, and Martin Paegert

Ghezzi et al. 2014 The Astronomical Journal 148 105.

  • Provider: AAS Journals

Caption: Figure 6.

Examples of the calibration for index 38 (see Table 4). Upper panel: Variation of the measured equivalent widths as a function of Teff, with the points color-coded by [Fe/H]. The dotted, solid, and dashed black lines represent Equation (1) for log g  = 4.44 and [Fe/H] = −0.50, 0.00, and +0.50, respectively. Lower panel: Variation of the measured equivalent widths as a function of [Fe/H], with the points color-coded by Teff. The dashed, solid, and dotted black lines represent Equation (1) for log g  = 4.44 and Teff  = 5000, 5750, and 6500 K, respectively. The calibration accurately represents the observed behavior of the points throughout the parameter space covered by the calibration sample.

(A color version and supplemental data of this figure are available in the online journal.)

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