220 citations · 1.3k across the 26 of their papers we have counts for
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Vision-Based Estimation of Small Body Rotational State during the Approach Phase
Paolo Panicucci, Jérémy Lebreton, Roland Brochard +2
The heterogeneity of the small body population complicates the prediction of small body properties before the spacecraft's arrival. In the context of autonomous small body explorat…
Image simulation for space applications with the SurRender software
Jérémy Lebreton, Roland Brochard, Matthieu Baudry +9
Image Processing algorithms for vision-based navigation require reliable image simulation capacities. In this paper we explain why traditional rendering engines may present limitat…
Exozodiacal clouds: Hot and warm dust around main sequence stars
Quentin Kral, Alexander V. Krivov, Denis Defrere +7
A warm/hot dust component (at temperature 300K) has been detected around 20% of stars. This component is called "exozodiacal dust" as it presents similarities with the z…
Light Scattering and Thermal Emission by Primitive Dust Particles in Planetary Systems
Hiroshi Kimura, Ludmilla Kolokolova, Aigen Li +1
This review focuses on numerical approaches to deducing the light-scattering and thermal-emission properties of primitive dust particles in planetary systems from astronomical obse…
Models of the Eta Corvi debris disk from the Keck Interferometer, Spitzer and Herschel
J. Lebreton, C. Beichman, G. Bryden +4
Debris disks are signposts of analogues to small body populations of the Solar System, often however with much higher masses and dust production rates. The disk associated with the…
An Unbiased Near-infrared Interferometric Survey for Hot Exozodiacal Dust
Steve Ertel, Jean-Charles Augereau, Olivier Absil +5
Exozodiacal dust is warm or hot dust found in the inner regions of planetary systems orbiting main sequence stars, in or around their habitable zones. The dust can be the most lumi…
First-light LBT nulling interferometric observations: warm exozodiacal dust resolved within a few AU of eta Corvi
D. Defrère, P. M. Hinz, A. J. Skemer +37
We report on the first nulling interferometric observations with the Large Binocular Telescope Interferometer (LBTI), resolving the N' band (9.81 - 12.41 um) emission around the ne…
Exo-zodi modelling for the Large Binocular Telescope Interferometer
Grant M. Kennedy, Mark C. Wyatt, Vanessa Bailey +18
Habitable zone dust levels are a key unknown that must be understood to ensure the success of future space missions to image Earth analogues around nearby stars. Current detection…
Herschel's "Cold Debris Disks": Background Galaxies or Quiescent Rims of Planetary Systems?
A. V. Krivov, C. Eiroa, T. Löhne +24
(abridged) Infrared excesses associated with debris disk host stars detected so far peak at wavelengths around ~100μm or shorter. However, six out of 31 excess sources in the Hersc…
An interferometric study of the Fomalhaut inner debris disk. III. Detailed models of the exozodiacal disk and its origin
J. Lebreton, R. van Lieshout, J. -C. Augereau +15
[Abridged] Debris disks are extrasolar analogs to the solar system planetesimal belts. The star Fomalhaut harbors a cold debris belt at 140 AU as well as evidence of a warm dust co…
Morphology of the very inclined debris disk around HD 32297
Anthony Boccaletti, Jean-Charles Augereau, Anne-Marie Lagrange +6
Direct imaging of circumstellar disks at high angular resolution is mandatory to provide morphological information that bring constraints on their properties, in particular the spa…