activity
20132019
most citedAsteroids' physical models from combined dense and sparse photometry and scaling of the YORP effect by the observed obliquity distribution

85 citations · 183 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.EP201929 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.EP201732 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.EP201732 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.EP20175 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.EP201385 cited

Asteroids' physical models from combined dense and sparse photometry and scaling of the YORP effect by the observed obliquity distribution

J. Hanuš, J. Ďurech, M. Brož +116

The larger number of models of asteroid shapes and their rotational states derived by the lightcurve inversion give us better insight into both the nature of individual objects and…