8.6k citations · 12.3k across the 77 of their papers we have counts for
77 papers
Physical Characterization of Asteroid (16583) Oersted Combining Stellar Occultation and Photometric Data
Josef Hanuš, Marco Delbo, Petr Pokorný +2
We report a successful observation of a stellar occultation by asteroid (16583) Oersted, enabling a detailed physical characterization of its shape, spin state, and surface propert…
An ancient L- type family associated to (460) Scania in the Middle Main Belt as revealed by Gaia DR3 spectra
Roberto Balossi, Paolo Tanga, Marco Delbo +2
Asteroid families are typically identified using hierarchical clustering methods (HCM) in the proper element phase space. However, these methods struggle with overlapping families,…
Palomar discovery and initial characterization of naked-eye long period comet C/2022 E3 (ZTF)
B. T. Bolin, F. J. Masci, D. A. Duev +11
Long-period comets are planetesimal remnants constraining the environment and volatiles of the protoplanetary disc. We report the discovery of hyperbolic long-period comet C/2022 E…
Gaia view of primitive inner-belt asteroid families: Searching for the origins of asteroids Bennu and Ryugu
Marco Delbo, Chrysa Avdellidou, Kevin J. Walsh
Near-Earth asteroids Ryugu and Bennu, were visited, characterised, and sampled by the Hayabusa2 and OSIRIS-REx missions: remote sensing data and sample return analysis showed that…
Extending Lunar Impact Flash Observations into the Daytime with Short-Wave Infrared
Daniel Sheward, Marco Delbo, Chrysa Avdellidou +7
Lunar impact flash (LIF) observations typically occur in R, I, or unfiltered light, and are only possible during night, targeting the night side of a 10-60% illumination Moon, whil…
Identification of a 4.3 billion year old asteroid family and planetesimal population in the Inner Main Belt
Salvatore Ferrone, Marco Delbo, Chrysa Avdellidou +4
After performing a reassessment of the known dynamical asteroid families in the inner main belt, we report a newly discovered ancient asteroid family with an estimated age of $4.3\…