Notes. The stellar effective temperature and metallicity have the same sources (already reported in Table A.1 and reiterated here for convenience), while the sources of the stellar radius are listed in Table A.1. The stellar ages listed in the last column were derived with the isochrone placement algorithm (see Sect. 5.1) except for GJ1214 and Trappist-1 for which the lower limits come from Berta et al. (2011) and Filippazzo et al. (2015), respectively. We note that the [Fe/H] given here is the photospheric iron abundance relative to solar and not the iron coronal abundance. References: 1. Bonomo et al. (2017); 2. Piaulet et al. (2021); 3. Lanotte et al. (2014); 4. Borsa et al. (2019); 5. Kosiarek et al. (2019); 6. Rice et al. (2019); 7. Bakos et al. (2010); 8. von Braun et al. (2011); 9. Gillon et al. (2014); 10. Turnbull (2015); 11. Gillon et al. (2017); 12. Tabernero et al. (2021); 13. Zhao et al. (2014); 14. Hébrard et al. (2013); 15. Turner et al. (2019); 16. Hartman et al. (2011); 17. Eigmüller et al. (2019); 18. Lam et al. (2017); 19. Ellis et al. (2021); 20. Barragán et al. (2022); 21. Bochanski et al. (2018); 22. Assumption, because no [Fe/H] estimate is available in the literature; 23. Nardiello et al. (2022); 24. Suárez Mascareño et al. (2021).