64 citations · 215 across the 9 of their papers we have counts for
10 papers
Extracting Asteroid Physical Properties from Vera C. Rubin Observatory Science Validation Survey Data: Rotational Periods, Colors, and Taxonomies
V. Carruba, S. Greenstreet, M. Mastropietro +7
The Vera C. Rubin Observatory will enable large-scale characterization of minor bodies through high-cadence, multi-band photometry. Early Science Validation (SV) observations from…
Identifying the population of stable resonant asteroids using large databases
Valerio Carruba, Safwan Aljbaae, Rita de Cassia Domingos +2
Large observational surveys, like those that will be conducted at the Vera C. Rubin Observatory, are expected to discover up to one million new asteroids in the first year of opera…
Machine Learning applied to asteroid dynamics
V. Carruba, S. Aljbaae, R. C. Domingos +2
Machine Learning (ML) is the branch of computer science that studies computer algorithms that can learn from data. It is mainly divided into supervised learning, where the computer…
The Rafita asteroid family
S. Aljbaae, V. Carruba, J. R. Masiero +2
The Rafita asteroid family is an S-type group located in the middle main belt, on the right side of the 3J:-1A mean-motion resonance. The proximity of this resonance to the family…
On the highly inclined leptokurtic asteroid families
V. Carruba, R. C. Domingos, S. Aljbaae +1
leptokurtic asteroid families are families for which the distribution of the normal component of the terminal ejection velocity field is characterized by a positive val…
On the oldest asteroid families in the main belt
V. Carruba, D. Nesvorný, S. Aljbaae +2
Asteroid families are groups of minor bodies produced by high-velocity collisions. After the initial dispersions of the parent bodies fragments, their orbits evolve because of seve…
Dynamical evolution of the Cybele asteroids
Valerio Carruba, David Nesvorný, Safwan Aljbaae +1
The Cybele region, located between the 2J:-1A and 5J:-3A mean-motion resonances, is adjacent and exterior to the asteroid main belt. An increasing density of three-body resonances…
Dynamical evolution of V-type photometric candidates in the outer Main-belt
Mariela E. Huaman, Valerio Carruba, Rita Cassia Domingos
V-type asteroids, characterized by two absorption bands at 1.0 and 2.0 , are usually thought to be portions of the crust of differentiated or partially differentiated bodies. M…
Dynamical evolution and chronology of the Hygiea asteroid family
V. Carruba, R. C. Domingos, M. E. Huaman +2
The asteroid (10) Hygiea is the fourth largest asteroid of the Main Belt, by volume and mass, and it is the largest member of its own family. Previous works investigated the long-t…
A multi-domain approach to asteroid families identification
V. Carruba, R. C. Domingos, D. Nesvorný +3
Previous works have identified families halos by an analysis in proper elements domains, or by using Sloan Digital Sky Survey-Moving Object Catalog data, fourth release (SDSS-MOC4)…