Showing 1–20 of 53 results
/ Date/ Name
Apr 7, 2011Exo--Zodiacal Dust Levels for Nearby Main Sequence StarsAug 15, 2022The discovery and characterization of a kilometre sized asteroid inside the orbit of VenusJul 21, 2018The HOSTS Survey for Exozodiacal Dust: Preliminary results and future prospectsAug 15, 2018Orbital characterization of GJ1108A system, and comparison of dynamical mass with model-derived mass for resolved binariesSep 9, 2020Preliminary estimates of the Zwicky Transient Facility 'Ayló'chaxnim asteroid population completenessJun 2, 1999Physical conditions in shocked regions of Orion from ground-based observations of H_2ODec 4, 2006Interferometric Observations of RS Ophiuchi and the Origin of the Near-IR EmissionJan 12, 2018The path towards high-contrast imaging with the VLTI: the Hi-5 projectJan 17, 2015First-light LBT nulling interferometric observations: warm exozodiacal dust resolved within a few AU of eta CorviSep 3, 2025A JWST/MIRI view of k Andromedae b: Refining its mass, age, and physical parametersOct 17, 2022Observing inside the coronagraphic regime with optimized single-mode nulling interferometrySep 12, 1998Submillimeter Imaging of NGC 891 with SHARCNov 21, 1998SHARC 350 Micron Mapping of the Galactic Center from the Caltech Submillimeter ObservatoryJan 19, 2021Large Interferometer For Exoplanets (LIFE): I. Improved exoplanet detection yield estimates for a large mid-infrared space-interferometer missionMar 29, 2018The HOSTS survey - Exozodiacal dust measurements for 30 starsAug 31, 2016SEEDS direct imaging of the RV-detected companion to V450 Andromedae, and characterization of the systemNov 15, 2012Direct Imaging Discovery of a `Super-Jupiter' Around the late B-Type Star Kappa AndFeb 28, 2012Discovery of Small-Scale Spiral Structures in the Disk of SAO 206462 (HD 135344B): Implications for the Physical State of the Disk from Spiral Density Wave TheorySep 13, 2012New Techniques for High-Contrast Imaging with ADI: the ACORNS-ADI SEEDS Data Reduction PipelineNov 14, 2012Subaru Imaging of Asymmetric Features in a Transitional Disk in Upper Scorpius