activity
20132026
most citedIntroducing the Eulalia and new Polana asteroid families: re-assessing primitive asteroid families in the inner Main Belt

150 citations · 411 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.EP2026

Dark asteroids exhibiting intermediate characteristics between C and X types

Sunao Hasegawa, Chrysa Avdellidou, Michael Marsset +8

Large main-belt asteroids with visible geometric albedos below 0.1 are predominantly classified within the C- and X-complex spectroscopic classes. C-type and dark X-type asteroids…

astro-ph.EP2026

Shape and spin axis determination of the Tianwen-2 target asteroid (469219) Kamo'oalewa from lightcurve inversion

Roberto Bonamico, Josef Hanuš, Marco Delbo

Near-Earth asteroid (469219) Kamo'oalewa is an Earth quasi-satellite, temporarily trapped in a 1:1 orbital resonance with our planet. Despite its dynamical relevance and the hypoth…

astro-ph.EP2017★ 40 cited

Spin states of asteroids in the Eos collisional family

J. Hanuš, M. Delbo', V. Alí-Lagoa +33

Eos family was created during a catastrophic impact about 1.3 Gyr ago. Rotation states of individual family members contain information about the history of the whole population. W…

astro-ph.EP2016★ 93 cited

Near-Earth asteroid (3200) Phaethon. Characterization of its orbit, spin state, and thermophysical parameters

J. Hanus, M. Delbo, D. Vokrouhlicky +15

The near-Earth asteroid (3200) Phaethon is an intriguing object: its perihelion is at only 0.14 au and is associated with the Geminid meteor stream. We aim to use all available dis…

astro-ph.EP2015★ 84 cited

New and updated convex shape models of asteroids based on optical data from a large collaboration network

J. Hanuš, J. Ďurech, D. A. Oszkiewicz +165

Asteroid modeling efforts in the last decade resulted in a comprehensive dataset of almost 400 convex shape models and their rotation states. This amount already provided a deep in…

astro-ph.IM2015★ 4 cited

THERMAP: a mid-infrared spectro-imager for space missions to small bodies in the inner solar system

O. Groussin, J. Licandro, J. Helbert +28

We present THERMAP, a mid-infrared (8-16 μm) spectro-imager for space missions to small bodies in the inner solar system, developed in the framework of the MarcoPolo-R asteroid sam…

astro-ph.EP2013★ 150 cited

Introducing the Eulalia and new Polana asteroid families: re-assessing primitive asteroid families in the inner Main Belt

Kevin J. Walsh, Marco Delbó, William F. Bottke +2

The so-called Nysa-Polana complex of asteroids is a diverse and widespread group. It appears to be two overlapping families of different asteroid taxonomies: (44) Nysa is an E-type…

astro-ph.EP2013★ 40 cited

Physical properties of B-type asteroids from WISE data

Víctor Alí-Lagoa, Julia de León, Javier Licandro +4

Aims: Our aim is to obtain more information about the physical nature of B-type asteroids and extend on the previous work by studying their physical properties derived from fitting…