Context. 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 space. However, there is growing evidence that some of the real families are larger than the corresponding cluster of objects in orbital elements, and there...
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October 2022 (v1)Journal articleUploaded on: December 4, 2022
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April 21, 2015 (v1)Journal article
International audience
Uploaded on: December 4, 2022 -
January 2018 (v1)Journal article
International audience
Uploaded on: December 4, 2022 -
November 2014 (v1)Journal article
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 Kepler space telescope and then validated thanks to a radial velocity :follow-up with the SOPHIE spectrograph. It orbits its host star with a period of 86,647661 d +/- 3 s and a high eccentricity of 0.772 +/-...
Uploaded on: February 28, 2023 -
November 2017 (v1)Journal article
International audience
Uploaded on: December 3, 2022 -
October 2021 (v1)Journal article
Context. Until recently, the 3D shape, and therefore density (when combining the volume estimate with available mass estimates), and surface topography of the vast majority of the largest (D ≥ 100 km) main-belt asteroids have remained poorly constrained. The improved capabilities of the SPHERE/ZIMPOL instrument have opened new doors into...
Uploaded on: December 4, 2022