Showing 21–40 of 136 results
/ Date/ Name
Jul 13, 2018ERIS: revitalising an adaptive optics instrument for the VLTJul 17, 2006Disks around young stars with VLTI/MIDIDec 18, 2025Maximizing the sensitivity of ELT to habitable worlds with a space-based starshadeJan 18, 2018SUPERSHARP - Segmented Unfolding Primary for Exoplanet Research via Spectroscopic High Angular Resolution PhotographyMar 4, 2017Evolution of protoplanetary disks from their taxonomy in scattered light: Group I vs. Group IIApr 9, 2018Finding and Characterizing Other Worlds: the Thermal-IR ELT OpportunityNov 8, 2024The GPU-based High-order adaptive OpticS TestbenchJul 27, 2012PynPoint: An Image Processing Package for Finding ExoplanetsJan 6, 2021BEAST begins: Sample characteristics and survey performance of the B-star Exoplanet Abundance StudyMar 20, 2021METIS: The Mid-infrared ELT Imager and SpectrographJul 5, 2013Can a planet explain different cavity sizes for small and large dust grains in transition disks?Dec 5, 2018Evolutionary models of cold and low-mass planets: Cooling curves, magnitudes, and detectabilityDec 31, 2019MIRACLES: atmospheric characterization of directly imaged planets and substellar companions at 4-5 $μ$m. I. Photometric analysis of $β$ Pic b, HIP 65426 b, PZ Tel B and HD 206893 BNov 25, 2019Disks Around T Tauri Stars with SPHERE (DARTTS-S) II: Twenty-one new polarimetric images of young stellar disksJun 4, 2019ISPY -- NaCo Imaging Survey for Planets around Young stars. Discovery of an M dwarf in the gap between HD 193571 and its debris ringSep 2, 2021Occulter to Earth: Prospects for studying Earth-like planets with the E-ELT and a space-based occulterMar 20, 2021PCS -- A Roadmap for Exoearth Imaging with the ELTSep 9, 2020MIRACLES: atmospheric characterization of directly imaged planets and substellar companions at 4-5 $μ$m. II. Constraints on the mass and radius of the enshrouded planet PDS 70 bSep 1, 2017Was Planet 9 captured in the Sun's natal star-forming region?Sep 1, 2017Retrieval Analysis of the Emission Spectrum of WASP-12b: Sensitivity of Outcomes to Prior Assumptions and Implications for Formation History