Showing 1–20 of 136 results
/ Date/ Name
Nov 10, 2009Search for very low-mass brown dwarfs and free-floating planetary-mass objects in TaurusJun 22, 2011Searching for Gas Giant Planets on Solar System Scales: VLT NACO/APP Observations of the Debris Disk Host Stars HD172555 and HD115892Feb 28, 2013A young protoplanet candidate embedded in the circumstellar disk of HD100546Aug 4, 2019Atmospheric characterization of terrestrial exoplanets in the mid-infrared: biosignatures, habitability & diversityJul 16, 2018Exoplanet science with a space-based mid-infrared nulling interferometerJul 17, 2017M Dwarf Exoplanet Surface Density Distribution: A Log-Normal Fit from 0.07-400 AUOct 26, 2006Dust rings and filaments around the isolated young star V1331 CygniDec 8, 2011Resolving the inner regions of the HD97048 circumstellar disk with VLT/NACO polarimetric differential imagingJun 6, 2011VLT/NACO Polarimetric Differential Imaging of HD100546 - Disk Structure and Dust Grain Properties between 10-140 AUMay 10, 2010A large, massive, rotating disk around an isolated young stellar objectApr 19, 2015High-contrast imaging constraints on gas giant planet formation - The Herbig Ae/Be star opportunityFeb 13, 2013Gaps in the HD169142 protoplanetary disk revealed by polarimetric imaging: Signs of ongoing planet formation?Dec 16, 2014Confirmation and characterization of the protoplanet HD100546 b - Direct evidence for gas giant planet formation at 50 auOct 9, 2020Europium as a lodestar: diagnosis of radiogenic heat production in terrestrial exoplanetsOct 12, 2020Physically constrained causal noise models for high-contrast imaging of exoplanetsSep 2, 2010First Results From VLT NACO Apodizing Phase Plate: 4-micron Images of the Exoplanet beta Pictoris bMar 16, 2012Direct imaging constraints on planet populations detected by microlensingMay 31, 2012Searching for young Jupiter analogs around AP Col: L-band high-contrast imaging of the closest pre-main sequence starMay 16, 2006FU Orionis - The MIDI/VLTI PerspectiveApr 3, 2014Direct detection of exoplanets in the 3 -- 10 micron range with E-ELT/METIS