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20112026
most citedCombining asteroid models derived by lightcurve inversion with asteroidal occultation silhouettes

127 citations · 1.5k across the 57 of their papers we have counts for

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Showing 2019Show all

5 papers · 1 filter

astro-ph.EP2019★ 27 cited

Inversion of asteroid photometry from Gaia DR2 and the Lowell Observatory photometric database

Josef Durech, Josef Hanus, Radim Vanco

Rotation properties (spin-axis direction and rotation period) and coarse shape models of asteroids can be reconstructed from their disk-integrated brightness when measured from var…

astro-ph.EP2019★ 17 cited

The shape of (7) Iris as evidence of an ancient large impact?

J. Hanuš, M. Marsset, P. Vernazza +35

Asteroid (7) Iris is an ideal target for disk-resolved imaging owing to its brightness (V7-8) and large angular size of 0.33 arcsec during its apparitions. Iris is believed t…

astro-ph.EP2019★ 26 cited

Closing the gap between Earth-based and interplanetary mission observations: Vesta seen by VLT/SPHERE

R. JL. Fétick, L. Jorda, P. Vernazza +34

Context. Over the past decades, several interplanetary missions have studied small bodies in situ, leading to major advances in our understanding of their geological and geophysica…

astro-ph.EP2019★ 90 cited

Asteroid pairs: a complex picture

P. Pravec, P. Fatka, D. Vokrouhlický +45

We studied 93 asteroid pairs. We estimated times elapsed since separation of pair members that are between 7*10^3 and a few 10^6 yr. We derived the rotation periods for all the pri…

astro-ph.EP2019★ 32 cited

The homogeneous internal structure of CM-like asteroid (41) Daphne

B. Carry, F. Vachier, J. Berthier +48

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 st…