activity
20032026
most citedFUSE Survey of the Local Interstellar Medium within 200 Parsec

114 citations · 875 across the 39 of their papers we have counts for

collaborators
Showing astro-ph.IMShow all

9 papers · 1 filter

astro-ph.IM2026

Exoplanet atmospheres and demographics in the 2040s

Jens Kammerer, Sydney Vach, Sylvestre Lacour +7

Direct observations of exoplanets probe the demographics and atmospheric composition of young self-luminous companions, yielding insight into their formation and early evolution hi…

astro-ph.IM2025

Exoplanets in reflected starlight with dual-field interferometry and a fifth Unit Telescope at VLTI

Óscar Carrión-González, Sylvestre Lacour, Mathias Nowak

In this white paper, we propose an upgrade to the Very Large Telescope Interferometer (VLTI) consisting of the addition of a new 8m Unit Telescope (UT5). The primary goal of this u…

astro-ph.IM2025

Hunting exomoons with a kilometric baseline interferometer

Thomas O. Winterhalder, Antoine Mérand, Sylvestre Lacour +3

Despite numerous search campaigns based on a diverse set of observational techniques, exomoons - prospective satellites of extrasolar planets - remain an elusive and hard-to-pin-do…

astro-ph.IM2024★ 1 cited

VLTI Unit Telescope coudé train vibration control upgrade for GRAVITY+

Romain Laugier, Julien Woillez, Denis Defrère +15

Scaling up interferometry to 8m collectors should smooth-out the optical piston perturbations and allow a slow fringe tracker to obtain high precision correction on faint targets.…

astro-ph.IM2014★ 3 cited

CubeSats as pathfinders for planetary detection: the FIRST-S satellite

S. Lacour, V. Lapeyrère, L. Gauchet +6

The idea behind FIRST (Fibered Imager foR a Single Telescope) is to use single-mode fibers to combine multiple apertures in a pupil plane as such as to synthesize a bigger aperture…

astro-ph.IM2014

The interferometric baselines and GRAVITY astrometric error budget

S. Lacour, F. Eisenhauer, S. Gillessen +9

GRAVITY is a new generation beam combination instrument for the VLTI. Its goal is to achieve microarsecond astrometric accuracy between objects separated by a few arcsec. This $10^…