K2-370 b: a strongly irradiated sub-Neptune transiting a very active solar-type star.

We report on the detailed characterization of K2-370 b, a transiting sub-Neptune on a 2.14-d orbit around the chromospherically active G-type dwarf HD 284521 (⁠|$T_\mathrm{eff} = 5662\pm 44$|  K, |$\lt \log R^\prime _{\rm HK}\gt =-4.49$|⁠). The system parameters are derived based on a global fit to K2, TESS and CHEOPS photometry, and HARPS-N and HARPS radial velocities (RVs). A Gaussian process regression analysis is performed simultaneously to the orbital fit of the RVs of K2-370 to effectively model the strong stellar rotation signal with a period of |$13.5\pm 0.05$|  d and measure the planetary RV signal with semi-amplitude |$K_{\rm b}=5.6\pm 0.7$|  m s |$^{-1}$|⁠. We find that K2-370 b has a radius of |$2.67\pm 0.05$|   |${\rm R}_{\rm{\oplus }}$| and a mass of |$11.1\pm 1.4$|   |${\rm M}_{\rm{\oplus }}$|⁠. With an estimated equilibrium temperature |$T_\mathrm{eq}\sim 1480$| K, K2-370 b is the second-hottest sub-Neptune with a highly precise mass determination around primaries with |$T_\mathrm{eff}\gt 5500$|  K. The resulting density of |$3.2\pm 0.4$|  g cm |$^{-3}$| implies that K2-370 b either retains a significant (⁠|$\sim 2~{{\ \rm per\ cent}}$| by mass) H-rich atmosphere or its interior contains a high (⁠|$\sim 40~{{\ \rm per\ cent}}$|⁠) water–mass fraction. [ABSTRACT FROM AUTHOR]