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

8 citations · 12 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.IM20231 cited

High-angular resolution and high-contrast VLTI observations from Y to L band with the Asgard instrumental suite

Marc-Antoine Martinod, Denis Defrère, Michael Ireland +17

The Very Large Telescope Interferometer is one of the most proficient observatories in the world for high angular resolution. Since its first observations, it has hosted several in…

astro-ph.IM20221 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.IM20228 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.IM20222 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…