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The planet-hosting subdwarf B star V 391 Pegasi is a hybrid pulsator. Astronomy and Astrophysics 564.
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Modelling of solar mesogranulation. Astronomy and Astrophysics 565.
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Large-scale horizontal flows in the solar photosphere V: Possible evidence for the disconnection of bipolar sunspot groups from their magnetic roots. Astronomy and Astrophysics 566.
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Helioseismology of sunspots: Confronting observations with three-dimensional MHD simulations of wave propagation. Solar Physics 572.
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f-mode interactions with thin flux tubes: the scattering matrix. Astrophysical Journal 579.
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High-resolution mapping of flows in the solar interior: Fully consistent OLA inversion of helioseismic travel times. Solar Physics