DOI,IST REx ID,Research Group,Title of publication
10.5281/ZENODO.17580178,20936,LiBu,Is a 1D perturbative method sufficient for asteroseismic modelling of β Cephei pulsators?
10.3847/1538-4357/ad4708,17326,LiBu,Detectability of axisymmetric magnetic fields from the core to the surface of oscillating post-main-sequence stars
10.1093/mnras/stae2053,18172,LiBu,Asteroseismic signatures of core magnetism and rotation in hundreds of low-luminosity red giants
10.1051/0004-6361/202449893,18904,LiBu,Measuring stellar surface rotation and activity with the PLATO mission. I. Strategy and application to simulated light curves
10.3847/2041-8213/ad6b29,18306,LiBu,Redshifted sodium transient near exoplanet transit
10.1051/0004-6361/202450918,18528,LiBu,Unveiling complex magnetic field configurations in red giant stars
10.1038/s41550-024-02304-w,17189,LiBu,Supergranular-scale solar convection not explained by mixing-length theory
10.5281/zenodo.12804810,22802,LiBu,MESA inlist file
10.48550/arXiv.2307.03237,13447,LiBu,Asteroseismology with the Roman galactic bulge time-domain survey
10.3847/1538-4357/acd118,13443,LiBu,"Magnetic activity evolution of solar-like stars. I. Sph–age relation derived from Kepler observations"
10.1051/0004-6361/202346832,14256,LiBu,Asymmetries of frequency splittings of dipolar mixed modes: A window on the topology of deep magnetic fields