Detecting deep axisymmetric toroidal magnetic fields in stars: The traditional approximation of rotation for differentially rotating deep spherical shells with a general azimuthal magnetic field
H. Dhouib, S. Mathis, L.A. Bugnet, T. Van Reeth, C. Aerts, Astronomy &; Astrophysics 661 (2022).

Magnetic signatures on mixed-mode frequencies: I. An axisymmetric fossil field inside the core of red giants
L.A. Bugnet, V. Prat, S. Mathis, A. Astoul, K. Augustson, R.A. García, S. Mathur, L. Amard, C. Neiner, Astronomy &; Astrophysics 650 (2021).

ROOSTER: A machine-learning analysis tool for Kepler stellar rotation periods
S.N. Breton, A.R.G. Santos, L.A. Bugnet, S. Mathur, R.A. García, P.L. Pallé, Astronomy &; Astrophysics 647 (2021).

Horizontal shear instabilities in rotating stellar radiation zones: II. Effects of the full Coriolis acceleration
J. Park, V. Prat, S. Mathis, L.A. Bugnet, Astronomy &; Astrophysics 646 (2021).

Surface rotation and photometric activity for Kepler targets. I. M and K main-sequence stars
A.R.G. Santos, R.A. García, S. Mathur, L.A. Bugnet, J.L. van Saders, T.S. Metcalfe, G.V.A. Simonian, M.H. Pinsonneault, The Astrophysical Journal Supplement Series 244 (2019).

Determining surface rotation periods of solar-like stars observed by the Kepler mission using machine learning techniques
S.N. Breton, L.A. Bugnet, A.R.G. Santos, A.L. Saux, S. Mathur, P.L. Palle, R.A. Garcia, ArXiv (n.d.).