19 Apr 2016: Rameau et al. (2016) "suggest that either two planets on moderately eccentric orbits or three to four
planets with inhomogeneous masses and orbital properties are possible."
(Galicher et al. 2014): The planet has a very red color probably due to high content of atmospheric dust.
(Rameau et al. 2013b): the semi-major axis is inferred by a projected distance of 55.7±2.5 AU.
Host star metallicity of directly imaged wide-orbit planets: implications for planet formation
SWASTIK C., BANYAI R., NARANG M., MANOJ P., SIVARANI T. et al.
Astron. J.
, 161
, 114
paperarxiv
K-Stacker, an algorithm to hack the orbital parameters of planets hidden in high-contrast imaging. First applications to VLT SPHERE multi-epoch observations
LE COROLLER H., NOWÁK M., DELORME P., CHAUVIN G., GRATTON R., et al.
Astron. & Astrophys.
, 639
, A113
paperarxiv
The Gemini Planet Imager Exoplanet Survey: Giant Planet and Brown Dwarf Demographics From 10-100 AU
NIELSEN E., DE ROSA R., MACINTOSH B., WANG J., RUFFIO J.-B. et al.
Astron. J.
, 158
, 13
paperarxiv
On the Mass Function, Multiplicity, and Origins of Wide-Orbit Giant Planets
WAGNER K., APAIL D. & KRATTER K.
ApJ
, accepted
arxiv
Two decades of Exoplanetary Science with Adaptive Optics
CHAUVIN, G.
SPIE Astronomical Telescopes and Instrumentation
arxivpaper
Constraining the presence of giant planets in two-belt debris disk systems with VLT/SPHERE direct imaging and dynamical arguments
MATTHEWS, E., HINKLEY, S., VIGAN, A., KENNEDY, G., SUTLIEFF, B. et al.
MNRAS
, 480
, 2757
paper
Investigating the young Solar System analog HD95086 - A combined HARPS and SPHERE exploration
CHAUVIN G., GRATTON R., BONNEFOY M., LAGRANGE A.-M., de BOER J. et al.
Astron. & Astrophys.
, 617
, A76
paperarxiv
Deep ALMA Search for CO Gas in the HD 95086 Debris Disc
BOOTH M., MATRA L., SU K., KRAL Q., HALES A. et al.
MNRAS
arxiv
ALMA 1.3 Millimeter Map of the HD 95086 System
SU K., MACGREGOR M., BOOTH M., WILNER D., FLAHERTY K., HUGHES M. et al.
Astron. J.
, accepted
arxiv
Space Technology for Directly Imaging and Characterizing Exo-Earths