Assessing the accuracy of the surface gravity determination in late-type stars with solar-like pulsators
Article first published online: 15 NOV 2011
© 2011 The Authors Monthly Notices of the Royal Astronomical Society © 2011 RAS
Monthly Notices of the Royal Astronomical Society: Letters
Volume 419, Issue 1, pages L34–L38, January 2012
How to Cite
Morel, T. and Miglio, A. (2012), Assessing the accuracy of the surface gravity determination in late-type stars with solar-like pulsators. Monthly Notices of the Royal Astronomical Society: Letters, 419: L34–L38. doi: 10.1111/j.1745-3933.2011.01172.x
- Issue published online: 13 DEC 2011
- Article first published online: 15 NOV 2011
- Accepted 2011 October 10. Received 2011 October 10; in original form 2011 September 7
Table S1. Mean effective temperature, iron content and surface gravities from the four different methods for the stars in Table 1. The error bars are the quadratic sum of the standard deviation of the individual measurements and the typical uncertainty in the parameter determination (80K for Teff, 0.1dex for [Fe/H], 0.1dex for the ionization and isochrone gravities, and 0.15dex for the strong-line gravities). The numbers in brackets are the number of measurements. The typical uncertainty in the seismic logg is 0.03dex (see text).
|MNL2_1172_sm_TableS1.dat||6K||Supporting info item|
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