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Cited article:

Monte Carlo simulation of solar p-mode profiles revisited: Bias and uncertainty estimation from one, not many, fits

T. Toutain, Y. Elsworth, W. J. Chaplin

A&A, 433 2 (2005) 713-715

Published online: 2005-03-22

DOI: https://doi.org/10.1051/0004-6361:20042508

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

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

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EFFICIENT PSEUDO-GLOBAL FITTING FOR HELIOSEISMIC DATA

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The Astrophysical Journal 694 (1) 144 (2009)
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On understanding the meaning of l = 2 and 3 p-mode frequencies as measured by various helioseismic instruments

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Asteroseismology of solar-type stars

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Living Reviews in Solar Physics 16 (1) (2019)
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