activity
20162026
most citedBroadband near-infrared astronomical spectrometer calibration and on-sky validation with an electro-optic laser frequency comb

47 citations · 99 across the 10 of their papers we have counts for

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Showing astro-ph.IMShow all

5 papers · 1 filter

astro-ph.IM2026

Non-common path aberration compensation and a dark hole loop with a pyramid adaptive optics system: Application to SAXO+

C. Goulas, R. Galicher, F. Vidal +16

In ground-based high-contrast instruments, non-common path aberrations (NCPAs) limit detection performance, as they are unseen by the adaptive optics (AO) wavefront sensor but impa…

astro-ph.IM2025

High-resolution, high-efficiency narrowband spectroscopy with an s-p-phased holographic grating in double pass

Casper Farret Jentink, Francesco Pepe, Christophe Lovis +3

High-resolution spectroscopy (R>50,000) in astronomy typically uses echelle-type spectrographs, which excel for exoplanet detection via radial velocity but compromise throughput fo…

astro-ph.IM2024★ 2 cited

Numerical simulations for the SAXO+ upgrade: Performance analysis of the adaptive optics system

Charles Goulas, Raphaël Galicher, Fabrice Vidal +16

SPHERE, operating at the VLT since 2014, is currently one of the high-contrast instruments with a higher performance. Its adaptive optics system, known as SAXO, will be upgraded to…

astro-ph.IM2022

NIRPS Front-End: Design, performance, and lessons learned

N. Blind, U. Conod, A. de Meideros +13

NIRPS (Near Infra-Red Planet Searcher) is an AO-assisted and fiber-fed spectrograph for high precision radial velocity measurements in the YJH-bands. NIRPS also has the specificity…

astro-ph.IM2016★ 7 cited

Adaptive optics for high resolution spectroscopy: A direct application with the future NIRPS spectrograph

Uriel Conod, Nicolas Blind, François Wildi +1

Radial velocity instruments require high spectral resolution and extreme thermo-mecanical stability, even more difficult to achieve in near-infra red (NIR) where the spectrograph h…