activity
20052026
most citedThe size, shape, density and ring of the dwarf planet Haumea from a stellar occultation

258 citations · 1.4k across the 40 of their papers we have counts for

collaborators
Showing 2017 · astro-ph.EPShow all

5 papers · 2 filters

astro-ph.EP2017★ 32 cited

Photometric survey, modelling, and scaling of long-period and low-amplitude asteroids

A. Marciniak, P. Bartczak, T. Müller +40

The available set of spin and shape modelled asteroids is strongly biased against slowly rotating targets and those with low lightcurve amplitudes. As a consequence of these select…

astro-ph.EP2017★ 5 cited

Shape and spin determination of Barbarian asteroids

M. Devogèle, P. Tanga, P. Bendjoya +51

Context. The so-called Barbarian asteroids share peculiar, but common polarimetric properties, probably related to both their shape and composition. They are named after (234) Barb…

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.EP2017★ 50 cited

Study of the plutino object (208996) 2003 AZ84 from stellar occultations: size, shape and topographic features

A. Dias-Oliveira, B. Sicardy, J. L. Ortiz +60

We present results derived from four stellar occultations by the plutino object (208996) 2003~AZ, detected at January 8, 2011 (single-chord event), February 3, 2012 (multi-c…

astro-ph.EP2017★ 46 cited

3D shape of asteroid (6)~Hebe from VLT/SPHERE imaging: Implications for the origin of ordinary H chondrites

M. Marsset, B. Carry, C. Dumas +15

Context. The high-angular-resolution capability of the new-generation ground-based adaptive-optics camera SPHERE at ESO VLT allows us to assess, for the very first time, the crater…