orbitize! is a powerful software package for Bayesian modeling of the orbital parameters of resolved binary objects from time series measurements, developed with the needs of the high-contrast imaging community in mind.
The Hubble Space Telescope's unique UV-optical capabilities are essential for understanding the early stages of galaxy assembly and the cosmic star formation history, complementing the infrared capabilities of the James Webb Space Telescope.
Three superfast rotating main-belt asteroids were discovered in a preliminary search of the DECam Ecliptic Exploration Project (DEEP) data, implying a higher incidence rate of such objects than previously measured.
Aquarius III is a newly discovered low-luminosity, metal-poor, and kinematically cold stellar system located in the outer halo of the Milky Way, likely on first infall.
Siril is a comprehensive, open-source software package that provides advanced tools for preprocessing and post-processing astronomical images, enabling users to produce high-quality images of celestial objects.
A T5-T6 brown dwarf at a distance of 1.8-2.3 kpc from the Sun, with evidence of low metallicity ([M/H] ≤ -0.5) and a high transverse velocity of 172-214 km/s, suggesting it is likely a member of the Milky Way thick disk or halo.
The updated catalogue of δ Scuti pulsators in binary systems contains over 1000 such objects, providing detailed statistical properties, correlations, and evolutionary diagrams of these stars.
The physical properties, including size, shape, absolute magnitude, and geometric albedo, of trans-Neptunian object (143707) 2003 UY117 were determined through a combination of stellar occultation observations and photometric measurements.
This work presents the largest extragalactic surveys at submillimeter wavelengths, combining the Herschel Redshift Survey (HeRS) and Herschel Large Mode Survey (HeLMS) to provide high-quality, consistent maps covering 360 square degrees near the celestial equator.
Three new outer satellites have been discovered around Uranus and Neptune through ultra-deep pencil beam surveys, revealing dynamical groupings of these distant irregular moons.