Context. Some Ap stars that have a strong enough magnetic field and a sufficiently low v sini
show spectral lines resolved into their magnetically split components. Aims. We present the …

We present the first results from the Transiting Exoplanet Survey Satellite (TESS) on the
rotational and pulsational variability of magnetic chemically peculiar A-type stars. We …

We present the first results of a volume-limited survey of main-sequence (MS) magnetic
chemically peculiar (mCP) stars. The sample consists of all identified intermediate-mass MS …

Strong magnetic fields in chemically peculiar A-type (Ap) stars typically suppress low-
overtone pressure modes (p modes) but allow high-overtone p modes to be driven. KIC …

We present the results of a systematic search for new rapidly oscillating Ap (roAp) stars
using the 2-min cadence data collected by the Transiting Exoplanet Survey Satellite (TESS) …

Kilonova spectra provide us with information of r-process nucleosynthesis in neutron star
mergers. However, it is still challenging to identify individual elements in the spectra mainly …

Context. Exoplanet properties crucially depend on the parameters of their host stars: more
accurate stellar parameters yield more accurate exoplanet characteristics. When the …

We report the identification of 61.45 d− 1 (711.2 μHz) oscillations, with amplitudes of 62.6
μmag, in KIC 4768731 (HD 225914) using Kepler photometry. This relatively bright (V= 9.17) …

Aims. The determination of effective temperature for chemically peculiar (CP) stars by means
of photometry is a sophisticated task due to their abnormal colours. Standard calibrations for …

Context. High spectral resolution studies of cool Ap stars reveal conspicuous anomalies of
the shape and strength of many absorption lines. This is a signature of large atmospheric …