L. Rodet

TL;DR: In this paper, the authors show how long-baseline interferometric observations guided by radial-velocity can be used in such a way to detect giant exoplanets.

TL;DR: In this paper, the presence and mass of an exoplanet can now be effectively derived from the astrometry of another ex-oplanet, using Markov chain Monte Carlo simulations in Jacobi coordinates.

TL;DR: In this article, the authors fit atmospheric models for giant planets and brown dwarfs and performed spectral retrievals with petitRADTRANS and ATMO on the observed GRAVITY, SPHERE, and GPI spectra of HD 206893 B.

TL;DR: The ExoGRAVITY project as discussed by the authors is a survey of known young giant exoplanets located in the range of 0.1" to 2" from their stars, where adaptive optics and interferometric observations results in a considerable contrast gain compared to single-telescope, extreme AO systems.