  Past studies have demonstrated that atmospheric escape by the core-powered
mass-loss mechanism can explain a multitude of observations associated with the
radius valley that separates the super-Earth and sub-Neptune planet
populations. Complementing such studies, in this work, we present a shortlist
of planets that could be losing their atmospheres today if their evolution is
indeed primarily dictated by core-powered mass-loss. We use Bayesian inference
analysis on our planet evolution and mass-loss model to estimate the posteriors
of the parameters that encapsulate the current state of a given planet, given
their published masses, radii and host star properties. Our models predict that
the following planets could be losing their atmospheres today at a rate
$\gtrsim 10^7$ g/s at 50\% confidence level: pi Men c, Kepler-60 d, Kepler-60
b, HD 86226 c, EPIC 249893012 b, Kepler-107 c, HD 219134 b, Kepler-80 e,
Kepler-138 d and GJ 9827 d. As a by-product of our Bayesian inference analysis,
we were also able to identify planets that most-likely harbor either secondary
atmospheres abundant with high mean-molecular weight species, low-density
interiors abundant with ices, or both. The planets belonging to this second
category are WASP-47 e, Kepler-78 b, Kepler-10 b, CoRoT-7 b, HD 80653 b, 55 Cnc
e and Kepler-36 b. While the aforementioned lists are by no means exhaustive,
we believe that candidates presented here can serve as useful input for target
selection for future surveys and for testing the importance of core-powered
mass-loss in individual planetary systems.
