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20112023
most citedCombining asteroid models derived by lightcurve inversion with asteroidal occultation silhouettes

127 citations · 439 across the 9 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.EP2020★ 42 cited

Precise astrometry and diameters of asteroids from occultations -- a data-set of observations and their interpretation

David Herald, David Gault, Robert Anderson +10

Occultations of stars by asteroids have been observed since 1961, increasing from a very small number to now over 500 annually. We have created and regularly maintain a growing dat…

astro-ph.EP2019★ 47 cited

Pluto's lower atmosphere and pressure evolution from ground-based stellar occultations, 1988-2016

E. Meza, B. Sicardy, M. Assafin +167

Context. Pluto's tenuous nitrogen (N2) atmosphere undergoes strong seasonal effects due to high obliquity and orbital eccentricity, and has been recently (July 2015) observed by th…

astro-ph.EP2017★ 103 cited

Volumes and bulk densities of forty asteroids from ADAM shape modeling

Josef Hanus, Matti Viikinkoski, Franck Marchis +11

Disk-integrated photometric data of asteroids do not contain accurate information on shape details or size scale. Additional data such as disk-resolved images or stellar occultatio…

astro-ph.EP2016★ 87 cited

Pluto's atmosphere from the 29 June 2015 ground-based stellar occultation at the time of the New Horizons flyby

B. Sicardy, J. Talbot, E. Meza +65

We present results from a multi-chord Pluto stellar occultation observed on 29 June 2015 from New Zealand and Australia. This occurred only two weeks before the NASA New Horizons f…

astro-ph.EP2011★ 127 cited

Combining asteroid models derived by lightcurve inversion with asteroidal occultation silhouettes

Josef Durech, Mikko Kaasalainen, David Herald +9

Asteroid sizes can be directly measured by observing occultations of stars by asteroids. When there are enough observations across the path of the shadow, the asteroid's projected…