Showing 41–60 of 1,412 results
/ Date/ Name
Jan 8, 2026Paving the Road to the Habitable Worlds Observatory with High-Resolution Imaging I: New and Archival Speckle Observations of Potential HWO Target StarsJan 1, 2026KMT-2024-BLG-0816/OGLE-2024-BLG-0519 -- A Microlensing Event with Candidate Free-Floating Planet Lens and Blended LightDec 17, 2025Characterising injection signatures in Jupiter's ultraviolet aurora using Juno observationsDec 16, 2025Why the Northern Hemisphere Needs a 30-40 m Telescope and the Science at Stake: Key Targets of Opportunity on Gas and Ice Giants and their satellitesDec 16, 2025The quest for Magrathea planets. II. Orbital stability of exoplanets formed around double white dwarfsDec 13, 2025Transients as Determinants of HabitabilityDec 13, 2025Toward the time-domain spectroscopic study of the dynamic life of stars: from accretion to magnetic activityDec 12, 2025JWST/NIRSpec Detects Warm CO Emission in the Terrestrial-Planet Zone of HD 131488Dec 8, 2025SPHEREx Pre-Perihelion Mapping of $\mathrm{H_2O}$, $\mathrm{CO_2}$, and $\mathrm{CO}$ in Interstellar Object 3I/ATLASDec 3, 2025Improving Accretion Diagnostics for Young Stellar Objects with Mid-infrared Hydrogen lines from JWST/MIRIDec 2, 2025Stellar chemistry and planet size: insights from GALAH DR4Dec 1, 2025SCExAO/CHARIS and Gaia Direct Imaging and Astrometric Discovery of a Superjovian Planet 3--4 lambda/D from the Accelerating Star HIP 54515Nov 25, 2025Tracking the Activity of the Interstellar Object 3I/ATLAS through its PerihelionNov 24, 2025Chemical and Isotopic Homogeneity Between the L Dwarf CD-35 2722 B and its Early M Host StarNov 21, 2025Kepler-1624b Has No Significant Transit Timing VariationsNov 17, 2025Thermal infrared characterization of spatially unresolved resident space objects: Prospects from analytical two-component modelingNov 7, 2025Are We There Yet? Challenges in Quantifying the Frequency of Earth Analogs in the Habitable ZoneNov 5, 2025A new broadband atmospheric dispersion corrector for HROS-TMTNov 4, 2025The First Occurrence Rate Estimates for Exoplanets in Small-Separation Binary Star Systems: Planet Occurrence is Suppressed in Binary StarsOct 29, 2025Tidally driven inertial waves enhance eccentricity damping and spin evolution in planets and stars