Showing 361–380 of 1,412 results
/ Date/ Name
Sep 6, 2023Revisiting Orbital Evolution in HAT-P-2 b and Confirmation of HAT-P-2 cSep 3, 2023KMT-2021-BLG-1547Lb: Giant microlensing planet detected through a signal deformed by source binarityAug 30, 2023An Astrometric Approach to Measuring the Color of an ObjectAug 29, 2023Water Condensation Zones around Main Sequence StarsAug 21, 2023Synergies between interstellar dust and heliospheric science with an Interstellar ProbeAug 15, 2023A large topographic feature on the surface of the trans-Neptunian object (307261) 2002 MS$_4$ measured from stellar occultationsAug 10, 2023First laboratory demonstration of real-time multi-wavefront sensor single conjugate adaptive opticsAug 10, 2023Source of radio emissions induced by the Galilean moons Io, Europa and Ganymede: in situ measurements by JunoAug 9, 2023Demonstration of Orbit Determination for LEO Objects using the Murchison Widefield ArrayAug 4, 2023JWST/NIRCam Coronagraphy of the Young Planet-hosting Debris Disk AU MicroscopiiAug 3, 2023Gravitational instability, spiral substructure, and modest grain growth in a typical protostellar disk: Modeling multi-wavelength dust continuum observation of TMC1AJul 27, 2023Chasing rainbows and ocean glints: Inner working angle constraints for the Habitable Worlds ObservatoryJul 26, 2023The first evidence of tidally induced activity in a brown dwarf-M dwarf pair: A Chandra study of the NLTT 41135/41136 systemJul 25, 2023Concluding remarks: Faraday Discussion on astrochemistry at high resolutionJul 24, 2023Ro-vibrational Spectroscopy of CI Tau -- Evidence of a Multi-Component Eccentric Disk Induced by a PlanetJul 23, 2023Chasing Nomadic Worlds: A New Class of Deep Space MissionsJul 21, 2023Retrieval of the dayside atmosphere of WASP-43b with CRIRES+Jul 21, 2023Age distribution of exoplanet host stars: Chemical and Kinematics age proxies from GAIA DR3Jul 16, 2023Evolution of Neptune at Near-Infrared Wavelengths from 1994 through 2022Jul 13, 2023Atmospheric composition of WASP-85Ab with ESPRESSO/VLT observations