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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 7.

Residuals (ΔEW = EWcalc–EWobs) from the calibrations of index 38 as a function of, from top to bottom, EWobs, Teff, [Fe/H], and log g. The horizontal black solid lines indicate the perfect agreement. The blue and red dashed lines show, respectively, the 1σ and 2σ limits, where σ = 18.36 mÅ  is the standard deviation of the residuals (see Section 4). The green dotted line in the upper panel represents the linear fit to the residuals, which has a correlation coefficient R2 = 0.007. In the panels for Teff, [Fe/H], and log g, the fit cannot be distinguished from the black line. No significant trends can be observed for the residuals as a function of the EWs and atmospheric parameters.

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