@article{12f6217e1bb74bd58aa60c93e468de74,
title = "A new correction of stellar oscillation frequencies for near-surface effects",
abstract = "Context. Space-based observations of solar-like oscillations present an opportunity to constrain stellar models using individual mode frequencies. However, current stellar models are inaccurate near the surface, which introduces a systematic difference that must be corrected.",
keywords = "Asteroseismology, Stars: individual: HD 52265, Stars: oscillations",
author = "Ball, {W. H.} and L. Gizon",
note = "Funding Information: W.H.B. and L.G. acknowledge research funding by Deutsche Forschungsgemeinschaft (DFG) under grant SFB 963/1 “Astrophysical flow instabilities and turbulence” (Project A18). L.G. also acknowledges support from EU FP7 Collaborative Project “Exploitation of Space Data for Innovative Helio- and Asteroseismology” (SPACEINN). Part of this work was completed during a visit to the Aarhus Stellar Astrophysics Centre.",
year = "2014",
month = aug,
day = "1",
doi = "10.1051/0004-6361/201424325",
language = "English (US)",
volume = "568",
journal = "Astronomy and Astrophysics",
issn = "0004-6361",
publisher = "EDP Sciences",
}