Proc. IAU volume 13, issue S334, P368-369 2017 DOI: 10.1017/s1743921317008808 View full text
Jesper Storm, Dariusz Graczyk, Marica Valentini, Friedrich Anders, Cristina Chiappini, Wolfgang Gieren, Grzegorz Pietrzynski

Abstract: AbstractThe Kepler and CoRoT satellites have determined precise asteroseismic radii for large samples of red giant stars. Combining these data with data from spectroscopic and photometric surveys has led to precise distance determinations using comprehensive Bayesian methods. Here we determine angular diameters and thus distances using the interferometrically calibrated near-IR surface-brightness method finding good agreement with previous results. The method can easily be reversed when accurate Gaia parallaxe…

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