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20102020
most citedSOPHIE velocimetry of Kepler transit candidates XII. KOI-1257 b: a highly eccentric three-month period transiting exoplanet

87 citations · 377 across the 8 of their papers we have counts for

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7 papers · 1 filter

astro-ph.EP2020★ 8 cited

Physical parameters of selected Gaia mass asteroids

E. Podlewska-Gaca, A. Marciniak, V. Alí-Lagoa +36

Thanks to the Gaia mission, it will be possible to determine the masses of approximately hundreds of large main belt asteroids with very good precision. We currently have diameter…

astro-ph.EP2017★ 32 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.EP2017★ 5 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.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.EP2014★ 87 cited

SOPHIE velocimetry of Kepler transit candidates XII. KOI-1257 b: a highly eccentric three-month period transiting exoplanet

A. Santerne, G. Hébrard, M. Deleuil +36

In this paper we report a new transiting warm giant planet: KOI-1257 b. It was first detected in photometry as a planet-candidate by the space telescope and then val…

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…