activity
20182026
most citedFirst on-sky demonstration of an integrated-photonic nulling-interferometer: The GLINT instrument

68 citations · 228 across the 32 of their papers we have counts for

collaborators
Showing 2022Show all

6 papers · 1 filter

astro-ph.IM2022★ 28 cited

Asgard/NOTT: L-band nulling interferometry at the VLTI I. Simulating the expected high-contrast performance

Romain Laugier, Denis Defrère, Benjamin Courtney-Barrer +13

Context: NOTT (formerly Hi-5) is a new high-contrast L' band (3.5-4.0 \textmu m) beam combiner for the VLTI with the ambitious goal to be sensitive to young giant exoplanets down t…

astro-ph.IM2022★ 16 cited

Achromatic design of a photonic tricoupler and phase shifter for broadband nulling interferometry

Teresa Klinner-Teo, Marc-Antoine Martinod, Peter Tuthill +3

Nulling interferometry is one of the most promising technologies for imaging exoplanets within stellar habitable zones. The use of photonics for carrying out nulling interferometry…

astro-ph.IM2022★ 1 cited

Design of the new CHARA instrument SILMARIL: pushing the sensitivity of a 3-beam combiner in the H- and K-bands

Cyprien Lanthermann, Theo ten Brummelaar, Peter Tuthill +5

Optical interferometry is a powerful technique to achieve high angular resolution. However, its main issue is its lack of sensitivity, compared to other observation techniques. Eff…

astro-ph.IM2022★ 8 cited

L-band nulling interferometry at the VLTI with Asgard/Hi-5: status and plans

Denis Defrère, Azzurra Bigioli, Colin Dandumont +34

Hi-5 is the L'-band (3.5-4.0 m) high-contrast imager of Asgard, an instrument suite in preparation for the visitor focus of the VLTI. The system is optimized for high-contrast a…

astro-ph.IM2022★ 2 cited

High spectral-resolution interferometry down to 1 micron with Asgard/BIFROST at VLTI: Science drivers and project overview

Stefan Kraus, Daniel Mortimer, Sorabh Chhabra +10

We present science cases and instrument design considerations for the BIFROST instrument that will open the short-wavelength (Y/J/H-band), high spectral dispersion (up to R=25,000)…

astro-ph.IM2022

High Contrast Imaging at the Photon Noise Limit with WFS-based PSF Calibration

Olivier Guyon, Barnaby Norris, Marc-Antoine Martinod +10

Speckle Noise is the dominant source of error in high contrast imaging with adaptive optics system. We discuss the potential for wavefront sensing telemetry to calibrate speckle no…