activity
20092026
most citedAn interferometric study of the Fomalhaut inner debris disk. III. Detailed models of the exozodiacal disk and its origin

72 citations · 118 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.EP2026

VLTI/MATISSE observations of the hot dust around Pictoris: Observing faint objects with MATISSE

P. Priolet, J. -C. Augereau, J. Milli +32

Context: Hot exozodiacal dust has been detected around approximately 20% of nearby main-sequence stars, indicating that it is a common feature of extrasolar planetary systems. Howe…

astro-ph.SR2026

A self-consistent orbital architecture for GG Tau A. I. Simultaneous orbital fitting of the hierarchical triple

A. Lacquement, H. Beust, G. Duchêne +4

GG Tau is a young triple system with the close pair, --, and , surrounded by a massive circumtriple disk with a large inner cavity difficult to explain in a bin…

astro-ph.EP2026

Dynamics of the TWA 7 planetary system and possibility of an additional planet

A. Lacquement, H. Beust, G. Duchêne +1

The debris disk surrounding the young star TWA 7 exhibits morphological features that tightly constrain its planetary architecture. JWST/MIRI observations have recently revealed a…

astro-ph.EP2026

Cold and eccentric: a high-spectral resolution view of 51 Eri b with VLT/HiRISE

A. Denis, A. Vigan, G. Chauvin +35

Discovered almost 10 years ago, the giant planet 51 Eridani b is one of the least separated (0.2 arcsec) and faintest (J = 19.74 mag) directly imaged exoplanets known to date. Its…

astro-ph.EP2025★ 6 cited

The ExoGRAVITY survey: A K-band spectral library of giant exoplanet and brown dwarf companions

J. Kammerer, T. O. Winterhalder, S. Lacour +106

Direct observations of exoplanet and brown dwarf companions with near-infrared interferometry, first enabled by the dual-field mode of VLTI/GRAVITY, provide unique measurements of…

astro-ph.EP2025

Dust populations from 30 to 1000 au in the debris disk of HD 120326

C. Desgrange, J. Milli, G. Chauvin +15

Context. To date, more than a hundred debris disks have been spatially resolved. Among them, the young system HD 120326 stands out, displaying different disk substructures on both…

astro-ph.EP2013★ 38 cited

Can eccentric debris disks be long-lived? A first numerical investigation and application to Reticuli

V. Faramaz, H. Beust, P. Thébault +13

Imaging of debris disks has found evidence for both eccentric and offset disks. One hypothesis is that these provide evidence for massive perturbers that sculpt the observed struct…

astro-ph.EP2013★ 72 cited

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…

astro-ph.IM2009★ 2 cited

Infrared Detection and Characterization of Debris Disks, Exozodiacal Dust, and Exoplanets: The FKSI Mission Concept

W. C. Danchi, R. K. Barry, B. Lopez +17

The Fourier-Kelvin Stellar Interferometer (FKSI) is a mission concept for a nulling interferometer for the near-to-mid-infrared spectral region. FKSI is conceived as a mid-sized st…