output
20062022
most citedFrequency of Solar-Like Systems and of Ice and Gas Giants Beyond the Snow Line from High-Magnification Microlensing Events in 2005-2008

349 citations

10 papers

astro-ph.EP2022★ 9 cited

Asteroid spin-states of a 4 Gyr collisional family

D. Athanasopoulos, J. Hanus, C. Avdellidou +29

Families of asteroids generated by the collisional fragmentation of a common parent body have been identified using clustering methods of asteroids in their proper orbital element…

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.EP2013★ 50 cited

An anisotropic distribution of spin vectors in asteroid families

J. Hanuš, M. Brož, J. Ďurech +11

Current amount of ~500 asteroid models derived from the disk-integrated photometry by the lightcurve inversion method allows us to study not only the spin-vector properties of the…

astro-ph.EP2013★ 85 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…

astro-ph.EP2012★ 235 cited

MOA-2011-BLG-293Lb: A test of pure survey microlensing planet detections

J. C. Yee, Y. Shvartzvald, A. Gal-Yam +10

Because of the development of large-format, wide-field cameras, microlensing surveys are now able to monitor millions of stars with sufficient cadence to detect planets. These new…

astro-ph.EP2011★ 183 cited

MOA-2009-BLG-387Lb: A massive planet orbiting an M dwarf

Virginie Batista, A. Gould, S. Dieters +25

We report the discovery of a planet with a high planet-to-star mass ratio in the microlensing event MOA-2009-BLG-387, which exhibited pronounced deviations over a 12-day interval,…