228 citations
- Max Planck Institute for Extraterrestrial PhysicsDE4 papers
- Adam Mickiewicz University in PoznańPL3 papers
- Centre National de la Recherche ScientifiqueFR3 papers
- The Open UniversityGB3 papers
- University of St AndrewsGB3 papers
- Uniwersytet Komisji Edukacji Narodowej w KrakowiePL3 papers
- 143-GnoscaCH2 papers
- Aix-Marseille UniversitéFR2 papers
- Charles UniversityCZ2 papers
- Deutsches Zentrum für Luft- und Raumfahrt e. V. (DLR)DE2 papers
- École Normale Supérieure - PSLFR2 papers
- European Space Astronomy CentreES2 papers
7 papers
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…
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…
The doubly eclipsing quintuple low-mass star system 1SWASP J093010.78+533859.5
M. E. Lohr, A. J. Norton, E. Gillen +6
Our discovery of 1SWASP J093010.78+533859.5 as a probable doubly eclipsing quadruple system containing a contact binary with P~0.23 d and a detached binary with P~1.31 d was announ…
A Window on Exoplanet Dynamical Histories: Rossiter-McLaughlin Observations of WASP-13b and WASP-32b
R. D. Brothwell, C. A. Watson, G. Hebrard +42
We present Rossiter-McLaughlin observations of WASP-13b and WASP-32b and determine the sky-projected angle between the normal of the planetary orbit and the stellar rotation axis (…
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…
Near-UV Absorption, Chromospheric Activity, and Star-Planet Interactions in the WASP-12 system
C. A. Haswell, L. Fossati, T. Ayres +15
We observed the extreme close-in hot Jupiter system WASP-12 with HST. Near-UV transits up to three times deeper than the optical transit of WASP-12b reveal extensive diffuse gas, e…