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Cited article:

Oscillation mode linewidths and heights of 23 main-sequence stars observed byKepler

T. Appourchaux, H. M. Antia, O. Benomar, et al.
Astronomy & Astrophysics 566 A20 (2014)

Oscillation mode linewidths of main-sequence and subgiant stars observed byKepler

T. Appourchaux, O. Benomar, M. Gruberbauer, et al.
Astronomy & Astrophysics 537 A134 (2012)

Distortion of the p-mode peak profiles by the solar-cycle frequency shifts: do we need to worry?

W. J. Chaplin, Y. Elsworth, R. New and T. Toutain
Monthly Notices of the Royal Astronomical Society 384 (4) 1668 (2008)

On understanding the meaning of l = 2 and 3 p-mode frequencies as measured by various helioseismic instruments

T. Appourchaux and W. J. Chaplin
Astronomy & Astrophysics 469 (3) 1151 (2007)