Here we present juliet, a versatile tool for the analysis of transits, radial velocities, or both.
juliet is built over many available tools for the modelling of transits, radial velocities, and …

Planet formation is generally described in terms of a system containing the host star and a
protoplanetary disk,–, of which the internal properties (for example, mass and metallicity) …

Open clusters and young stellar associations are attractive sites to search for planets and to
test theories of planet formation, migration, and evolution. We present our search for, and …

Theories of the formation and early evolution of planetary systems postulate that planets are
born in circumstellar disks, and undergo radial migration during and after dissipation of the …

We report the discovery of TOI 837b and its validation as a transiting planet. We characterize
the system using data from the NASA Transiting Exoplanet Survey Satellite mission, the ESA …

Ultra-short period (USP) planets are a class of low-mass planets with periods shorter than
one day. Their origin is still unknown, with photo-evaporation of mini-Neptunes and in situ …

Poking the Beehive from Space: K2 Rotation Periods for Praesepe - IOPscience This site uses
cookies. By continuing to use this site you agree to our use of cookies. To find out more, see …

We present a precise characterization of the TOI-561 planetary system obtained by
combining previously published data with TESS and CHEOPS photometry, and a new set of …

ABSTRACT HD 179070, aka Kepler-21, is a V= 8.25 F6IV star and the brightest exoplanet
host discovered by Kepler. An early detailed analysis by Howell et al. of the first 13 months …

Planets in young clusters are powerful probes of the evolution of planetary systems. Here we
report the discovery of three planets transiting EPIC 247589423, a late-K dwarf in the …