Showing 1–20 of 124 results
/ Date/ Name
Feb 28, 2013A young protoplanet candidate embedded in the circumstellar disk of HD100546Aug 4, 2019Atmospheric characterization of terrestrial exoplanets in the mid-infrared: biosignatures, habitability & diversityNov 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 HD115892Jul 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