Tally of exoplanet-host stars showing a seismic signal

Most studies of exoplanets rely on precise stellar parameters. An attractive way to obtain these is through asteroseismology, provided the host star shows oscillations that can be analysed. However, both the number of detected exoplanets and the number of pulsating/oscillating stars are rising continuously, causing an updated list of seismic host stars and their properties to be overdue. As a consequence, we are now assembling this updated catalogue of pulsating/oscillating stars that host confirmed and/or candidate exoplanets, and we need your help to ensure that we have included your asteroseismic host star in the sample. We will revisit the seismic detection of the solar-like oscillators and perform grid-based modelling of stars in the sample using the BASTA code.