activity
20072026
most citedNew determination of the size and bulk density of the binary asteroid 22 Kalliope from observations of mutual eclipses

73 citations · 290 across the 12 of their papers we have counts for

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Showing astro-ph.EPShow all

5 papers · 1 filter

astro-ph.EP2025★ 2 cited

Asteroid sizes determined with thermophysical model and stellar occultations

A. Choukroun, A. Marciniak, J. Ďurech +165

Context. The sizes of many asteroids, especially slowly rotating, low-amplitude targets, remain poorly constrained due to selection effects. These biases limit the availability of…

astro-ph.EP2019★ 29 cited

Thermal properties of slowly rotating asteroids: Results from a targeted survey

A. Marciniak, V. Alí-Lagoa, T. G. Müller +51

Context. Earlier work suggests that slowly rotating asteroids should have higher thermal inertias than faster rotators because the heat wave penetrates deeper into the sub-surface.…

astro-ph.EP2017★ 32 cited

Against the biases in spins and shapes of asteroids

A. Marciniak, F. Pilcher, D. Oszkiewicz +21

Physical studies of asteroids depend on an availability of lightcurve data. Targets that are easy to observe and analyse naturally have more data available, so their synodic period…

astro-ph.EP2015★ 17 cited

The non-convex shape of (234) Barbara, the first Barbarian

P. Tanga, B. Carry, F. Colas +37

Asteroid (234) Barbara is the prototype of a category of asteroids that has been shown to be extremely rich in refractory inclusions, the oldest material ever found in the Solar Sy…

astro-ph.EP2010★ 56 cited

Physical properties of ESA Rosetta target asteroid (21) Lutetia: Shape and flyby geometry

B. Carry, M. Kaasalainen, C. Leyrat +22

Aims. We determine the physical properties (spin state and shape) of asteroid (21) Lutetia, target of the ESA Rosetta mission, to help in preparing for observations during the flyb…