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20092022
most citedTriplicity and Physical Characteristics of Asteroid (216) Kleopatra

109 citations · 399 across the 10 of their papers we have counts for

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astro-ph.EP2022★ 20 cited

Constraints on the structure and seasonal variations of Triton's atmosphere from the 5 October 2017 stellar occultation and previous observations

J. Marques Oliveira, B. Sicardy, A. R. Gomes-Júnior +234

A stellar occultation by Neptune's main satellite, Triton, was observed on 5 October 2017 from Europe, North Africa, and the USA. We derived 90 light curves from this event, 42 of…

astro-ph.EP2019★ 16 cited

The trans-Neptunian object (84922) 2003 VS2 through stellar occultations

Gustavo Benedetti-Rossi, P. Santos-Sanz, J. L. Ortiz +50

We present results from three world-wide campaigns that resulted in the detections of two single-chord and one multi-chord stellar occultations by the Plutino object (84922) 2003~V…

astro-ph.EP2017★ 42 cited

The structure of Chariklo's rings from stellar occultations

D. Bérard, B. Sicardy, J. I. B. Camargo +79

Two narrow and dense rings (called C1R and C2R) were discovered around the Centaur object (10199) Chariklo during a stellar occultation observed on 2013 June 3. Following this disc…

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.EP2010★ 109 cited

Triplicity and Physical Characteristics of Asteroid (216) Kleopatra

Pascal Descamps, F. Marchis, J. Berthier +16

To take full advantage of the September 2008 opposition passage of the M-type asteroid (216) Kleopatra, we have used near-infrared adaptive optics (AO) imaging with the W.M. Keck I…

astro-ph.EP2009★ 36 cited

New insights on the binary asteroid 121 Hermione

P. Descamps, F. Marchis, J. Durech +29

We report on the results of a six-month photometric study of the main-belt binary C-type asteroid 121 Hermione, performed during its 2007 opposition. We took advantage of the rare…