Abstract The Jupiter Trojans, being trapped around the stable L4 and L5 Jupiter Lagrangian
points, are thought to be more primitive than the Main Belt asteroids. They are believed to …

Basaltic V-type asteroids are common in the inner part of the Main Asteroid Belt and much
less abundant in the mid and outer parts. They are of scientific interest because they sample …

Context. The sample of Solar system objects has dramatically increased over the last
decade. The number of measured properties (eg, diameter, taxonomy, rotation period …

The K2 mission of the Kepler Space Telescope allowed the observations of light curves of
small solar system bodies throughout the whole solar system. In this paper, we present the …

Context. The Asteroid Terrestrial-impact Last Alert System (ATLAS) is an all-sky survey
primarily aimed at detecting potentially hazardous near-Earth asteroids. Apart from the …

We present new thermophysical model fits of 1847 asteroids, deriving thermal inertia,
diameter, and Bond and visible geometric albedo. We use thermal flux measurements …

Context. Information about the spin state of asteroids is important for our understanding of
the dynamical processes affecting them. However, spin properties of asteroids are known for …

Context. CM-like asteroids (Ch and Cgh classes) are a major population within the broader
C-complex, encompassing about 10% of the mass of the main asteroid belt. Their internal …

We present V-band photometry of the 20 000 brightest asteroids using data from the All-Sky
Automated Survey for Supernovae (ASAS-SN) between 2012 and 2018. We were able to …

Context. Recent results for asteroid rotation periods from the TESS mission showed how
strongly previous studies have underestimated the number of slow rotators, revealing the …