Fig. 2 from Improving Stellar and Planetary Parameters of Transiting Planet Systems: The Case of TrES‐2

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Improving Stellar and Planetary Parameters of Transiting Planet Systems: The Case of TrES‐2

Authors: Alessandro Sozzetti, Guillermo Torres, David Charbonneau, David W. Latham, Matthew J. Holman, Joshua N. Winn, John B. Laird, and Francis T. O'Donovan

Sozzetti et al. 2007 The Astrophysical Journal 664 1190.

Provider: AAS Journals

Caption: Fig. 2.

Top: A 10 Å region of the Keck template spectrum of TrES‐2 centered on the Ca II H line. Bottom: A portion of the same spectrum containing the Li I line at 6707.8 Å (filled dots), compared to three synthetic profiles (lines of various colors and styles), each differing only in the lithium abundance assumed.

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