Showing 221–240 of 1,412 results
/ Date/ Name
Jul 30, 2024Obliquity Constraints for the Extremely Eccentric Sub-Saturn Kepler-1656 bJul 30, 2024Atmospheric characterization of the super-Jupiter HIP 99770 b with KPICJul 30, 2024TOI-757 b: an eccentric transiting mini-Neptune on a 17.5-d orbitJul 26, 2024A Data-driven Spectral Model of Main Sequence Stars in Gaia DR3Jul 24, 2024What is your favorite transient event? SOXS is almost ready to observe!Jul 23, 2024Exo-NINJA at Subaru: fiber-fed spectro-imaging of exoplanets and circumstellar disks at R$\sim$4000Jul 23, 2024Hints of planet formation signatures in a large-cavity disk studied in the AGE-PRO ALMA Large ProgramJul 22, 2024Gemini Planet Imager Observations of a Resolved Low-Inclination Debris Disk Around HD 156623Jul 19, 2024Formation and desorption of sulfur chains (H$_2$S$_x$ and S$_x$) in cometary ice: effects of ice composition and temperatureJul 17, 2024Size, albedo and rotational period of the Hayabusa2# target (98943) 2001 CC21Jul 16, 2024Fate of a remnant solid disk around an eccentric giant planetJul 14, 2024Inhomogeneous terminators on the exoplanet WASP-39 bJul 11, 2024L-band nulling interferometry at the VLTI with Asgard/NOTT: status and plansJul 10, 2024Sulphur dioxide in the mid-infrared transmission spectrum of WASP-39bJul 10, 2024Evidence for auroral influence on Jupiter's nitrogen and oxygen chemistry revealed by ALMAJul 3, 2024BOWIE-ALIGN: A JWST comparative survey of aligned vs misaligned hot Jupiters to test the dependence of atmospheric composition on migration historyJun 28, 2024High-energy spectra of LTT 1445A and GJ 486 reveal flares and activityJun 27, 2024The Space Coronagraph Optical Bench (SCoOB): 5. End-to-end simulations of polarization aberrationsJun 26, 2024The Incompressible Magnetohydrodynamic Energy Cascade Rate Upstream of Mars: Effects of the Total Energy and the Cross-Helicity on Solar Wind TurbulenceJun 25, 2024Revising Properties of Planet-Host Binary Systems. IV. The Radius Distribution of Small Planets in Binary Star Systems is Dependent on Stellar Separation