Showing 201–220 of 1,412 results
/ Date/ Name
Sep 24, 2024Tidally Heated Sub-Neptunes, Refined Planetary Compositions, and Confirmation of a Third Planet in the TOI-1266 SystemSep 23, 2024The Palomar twilight survey of 'Ayló'chaxnim, Atiras, and cometsSep 16, 2024Identifying activity induced RV periodicities and correlations using Central Line MomentsSep 10, 2024New evidence supporting past dust ejections from active asteroid (4015) Wilson-HarringtonSep 9, 2024Simulated performance of energy-resolving detectors towards exoplanet imaging with the Habitable Worlds ObservatorySep 5, 2024TOI-3568 b: a super-Neptune in the sub-Jovian desertSep 3, 2024Orbital Architectures of Planet-Hosting Binaries III. Testing Mutual Inclinations of Stellar and Planetary Orbits in Triple-Star SystemsSep 3, 2024A broad set of solar and cosmochemical data indicates high C-N-O abundances for the solar systemSep 1, 2024The GAPS Programme at TNG. LXI. Atmospheric parameters and elemental abundances of TESS young exoplanet host starsAug 28, 2024Atmospheric retrievals suggest the presence of a secondary atmosphere and possible sulfur species on L 98-59 d from JWST NIRSpec G395H transmission spectroscopyAug 27, 2024The Way To Circumbinary PlanetsAug 26, 2024SO as shock tracer in protoplanetary disks: the AB Aurigae caseAug 21, 2024A JWST MIRI MRS View of the $η$ Tel Debris Disk and its Brown Dwarf CompanionAug 19, 2024RV measurements of directly imaged brown dwarf GQ Lup B to search for exo-satellitesAug 19, 2024Fringing analysis and forward modeling of Keck Planet Imager and Characterizer (KPIC) spectraAug 14, 2024The $\sim$50-Myr-Old TOI-942c is Likely on an Aligned, Coplanar Orbit and Losing MassAug 13, 2024Deepest limits on scattered light emission from the Epsilon Eridani inner debris disk with HST/STISAug 10, 2024Mass determination of two Jupiter-sized planets orbiting slightly evolved stars: TOI-2420 b and TOI-2485 bAug 7, 2024A Survey of Protoplanetary Disks Using the Keck/NIRC2 Vortex CoronagraphAug 1, 2024Photoevaporation of protoplanetary discs with PLUTO+PRIZMO I. Lower X-ray-driven mass-loss rates due to enhanced cooling