2 papers
astro-ph.EP2024
Unsigned magnetic flux proxy from solar optical intensity spectra
F. Lienhard, A. Mortier, H. M. Cegla +3
The photospheric unsigned magnetic flux has been shown to be highly correlated with radial velocity (RV) variations caused by solar surface activity. This activity indicator is the…
astro-ph.EP2024
Characterisation of the TOI-421 planetary system using CHEOPS, TESS, and archival radial velocity data
A. F. Krenn, D. Kubyshkina, L. Fossati +88
The TOI-421 planetary system contains two sub-Neptune-type planets and is a prime target to study the formation and evolution of planets and their atmospheres. The inner planet is…