HR 95086
Data taken with the commissionning of the Gemini Planet Imager instrument were released to the community. I and my co-authors used these data to confirm the planet status of HR 95086 b and characterize it. From photometry, the planet Teff is 600-1500K and log g is 2.1-4.5. Evolutionary models yield a mass of 4-14MJup for a wide range of plausible initial conditions (Sinit = 8-13 kB/baryon). A&A paper. (Click on figures to enlarge)
Top: GPI images of the exoplanet HR 95086 b at H- and K1-band. Bottom left: Astrometric diagram comparing HR 95086 b motion and a putative background source. Bottom right: L' vs H-L' diagram with known exoplanets, L, T, and M-dwarfs.