Not exact matches
Revising the properties of the associated
planet candidates based on the updated host star characteristics and refitting the transit photometry, we find that our sample contains 20
planets or
planet candidates with radii smaller than 1.25 Earth radii, 20 super-Earths (1.25 - 2 Earth radii), 20 small Neptunes (2 - 4 Earth radii), three large Neptunes (4 - 6 Earth radii), and eight
giant planets (> 6 Earth radii).
A comparison with stellar properties in the
planet -
candidate catalog by Batalha et al. shows that radii for subgiants and
giants obtained from spectroscopic follow - up are systematically too low by up to a factor of 1.5, while the properties for unevolved stars are in good agreement.
Using the revised stellar properties, we recalculate the radii for 107
planet candidates in our sample, and comment on
candidates for which the radii change from a previously
giant -
planet / brown - dwarf / stellar regime to a sub-Jupiter size, or vice versa.
What remains to be found among the
Giant Planets like Jupiter and Saturn are some
candidates that combine all three ingredients for primitive life: energy, liquid water and some atmosphere.