activity
20082026
most citedCalibration of quasi-static aberrations in exoplanet direct-imaging instruments with a Zernike phase-mask sensor

158 citations · 1.4k across the 79 of their papers we have counts for

collaborators
Showing astro-ph.IMShow all

70 papers · 1 filter

astro-ph.IM2026

The Roman Coronagraph Community Participation Program: Using the Zernike wavefront sensor for a full characterisation of the Roman Space Telescope and the Coronagraph Instrument

Arthur Vigan, Alexis Bidot, Vincent Chambouleyron +4

The Roman Space Telescope Coronagraph Instrument (CGI) will demonstrate a series of technologies and techniques to enable the direct detection of reflected-light planets with space…

astro-ph.IM2026

Impact of segmented deformable mirrors on high-contrast testbeds for exoplanet imaging with future large space telescopes: contrast stability assessment on the HiCAT bench

Benjamin Buralli, Mamadou N'Diaye, Raphaël Pourcelot +13

We investigate the stability of a segmented deformable mirror (DM) on high-contrast testbeds and its impact on the images produced with coronagraphs. Segmented apertures are promis…

astro-ph.IM2024★ 3 cited

Cascade adaptive optics with a second stage based on a Zernike wavefront sensor for exoplanet observations

M. N'Diaye, A. Vigan, B. Engler +7

Over the past decade, the high-contrast observation of disks and gas giant planets around nearby stars has been made possible on ground-based instruments using extreme adaptive opt…

astro-ph.IM2024★ 3 cited

High-contrast imager for complex aperture telescopes (HiCAT): 8. Dark zone demonstration with simultaneous closed-loop low-order wavefront sensing and control

Rémi Soummer, Emiel H. Por, Raphaël Pourcelot +27

We present recent laboratory results demonstrating high-contrast coronagraphy for the future space-based large IR/Optical/Ultraviolet telescope recommended by the Decadal Survey. T…

astro-ph.IM2024★ 1 cited

High-contrast imager for complex aperture telescopes (HiCAT): 11. System-level demonstration of the Apodized Pupil Lyot Coronagraph with a segmented aperture in air

Rémi Soummer, Raphaël Pourcelot, Emiel H. Por +16

We present the final results of the Apodized Pupil Lyot Coronagraph (APLC) on the High-contrast imager for Complex Aperture Telescopes (HiCAT) testbed, under NASA's Strategic Astro…

astro-ph.IM2024

Mid-order wavefront control for exoplanet imaging: preliminary characterization of the segmented deformable mirror and Zernike wavefront sensor on HiCAT

B. Buralli, M. N'Diaye, R. Pourcelot +13

We study a mid-order wavefront sensor (MOWFS) to address fine cophasing errors in exoplanet imaging with future large segmented aperture space telescopes. Observing Earth analogs a…

astro-ph.IM2023

V(WF)S: Very Wide Field WaveFront Sensor for GLAO

Olivier Lai, Mark Chun, Stefan Kuiper +7

Adaptive optics is a technique mostly used on large telescopes. It turns out to be challenging for smaller telescopes (0.5~2m) due to the small isoplanatic angle, small subaperture…

astro-ph.IM2023

Exoplanet imaging with ELTs: exploring a second-stage AO with a Zernike wavefront sensor on the ESO/GHOST testbed

Mamadou N'Diaye, Arthur Vigan, Byron Engler +6

We propose to explore a cascade extreme Adaptive optics (ExAO) approach with a second stage based on a Zernike wavefront sensor (ZWFS) for exoplanet imaging and spectroscopy. Most…

astro-ph.IM2023★ 2 cited

Integrated photonic-based coronagraphic systems for future space telescopes

Niyati Desai, Lorenzo König, Emiel Por +38

The detection and characterization of Earth-like exoplanets around Sun-like stars is a primary science motivation for the Habitable Worlds Observatory. However, the current best te…

astro-ph.IM2023★ 1 cited

First light of VLT/HiRISE: High-resolution spectroscopy of young giant exoplanets

A. Vigan, M. El Morsy, M. Lopez +46

A major endeavor of this decade is the direct characterization of young giant exoplanets at high spectral resolution to determine the composition of their atmosphere and infer thei…

astro-ph.IM2023★ 4 cited

High-contrast detection of exoplanets with a kernel-nuller at the VLTI

Peter Marley Chingaipe, Frantz Martinache, Nick Cvetojevic +5

Context: The conventional approach to direct imaging has been the use of a single aperture coronagraph with wavefront correction via extreme adaptive optics. Such systems are limit…

astro-ph.IM2023★ 6 cited

Low-order wavefront control using a Zernike sensor through Lyot coronagraphs for exoplanet imaging: II. Concurrent operation with stroke minimization

R. Pourcelot, E. H. Por, M. N'Diaye +16

Wavefront sensing and control (WFSC) will play a key role in improving the stability of future large segmented space telescopes while relaxing the thermo-mechanical constraints on…

astro-ph.IM2022★ 5 cited

APLC-Optimization: an apodized pupil Lyot coronagraph design survey toolkit

Bryony F. Nickson, Emiel H. Por, Meiji M. Nguyen +9

We present a publicly available software package developed for exploring apodized pupil Lyot coronagraph (APLC) solutions for various telescope architectures. In particular, the pa…

astro-ph.IM2022★ 4 cited

HARMONI at ELT: A Zernike wavefront sensor for the high-contrast module -- Testbed results with realistic observation conditions

Adrien Hours, Alexis Carlotti, David Mouillet +10

ELT-HARMONI is the first light visible and near-IR integral field spectrograph (IFS) for the ELT. It covers a large spectral range from 450nm to 2450nm with resolving powers from 3…

astro-ph.IM2022★ 1 cited

Redundant Apodized Pupils (RAP) for high-contrast imagers robust to segmentation-due aberrations and island effects

Lucie Leboulleux, Alexis Carlotti, Mamadou N'Diaye +6

The imaging and characterization of a larger range of exoplanets, down to young Jupiters and exo-Earths will require accessing very high contrasts at small angular separations with…

astro-ph.IM2022

Statistical tests with multi-wavelength Kernel-phase analysis for the detection and characterization of planetary companions

Mamadou N'Diaye, David Mary, Frantz Martinache +4

Kernel phase is a method to interpret stellar point source images by considering their formation as the analytical result of an interferometric process. Using Fourier formalism, th…

astro-ph.IM2022★ 1 cited

Connecting SPHERE and CRIRES+ for the characterisation of young exoplanets at high spectral resolution: status update of VLT/HiRISE

A. Vigan, M. Lopez, M. El Morsy +32

New generation exoplanet imagers on large ground-based telescopes are highly optimised for the detection of young giant exoplanets in the near-infrared, but they are intrinsically…

astro-ph.IM2022★ 2 cited

3-beam self-calibrated Kernel nulling photonic interferometer

Nick Cvetojevic, Frantz Martinache, Peter Chingaipe +6

The use of interferometric nulling for the direct characterization of extrasolar planets is an exciting prospect, but one that faces many practical challenges when deployed on tele…

astro-ph.IM2022★ 3 cited

Redundant apodization for direct imaging of exoplanets 2: Application to island effects

Lucie Leboulleux, Alexis Carlotti, Mamadou N'Diaye +6

Telescope pupil fragmentation from spiders generates specific aberrations observed at various telescopes and expected on the large telescopes under construction. This so-called isl…

astro-ph.IM2022

Low-order wavefront control using a Zernike sensor through Lyot coronagraphs for exoplanet imaging

R. Pourcelot, M. N'Diaye, E. H. Por +19

Combining large segmented space telescopes, coronagraphy and wavefront control methods is a promising solution to produce a dark hole (DH) region in the coronagraphic image of an o…

astro-ph.IM2022★ 3 cited

Redundant apodization for direct imaging of exoplanets I: Robustness to primary mirror segmentation-induced errors outside the segment diffraction limit

Lucie Leboulleux, Alexis Carlotti, Mamadou N'Diaye

Direct imaging and spectroscopy of Earth-like planets and young Jupiters require contrasts up to 10^6-10^10 at angular separations of a few dozen milliarcseconds. To achieve this g…

astro-ph.IM2022★ 16 cited

Calibration of quasi-static aberrations in exoplanet direct-imaging instruments with a Zernike phase-mask sensor. IV. Temporal stability of non-common path aberrations in VLT/SPHERE

A. Vigan, K. Dohlen, M. N'Diaye +12

Coronagraphic imaging of exoplanets using ground-based instruments on large telescopes is intrinsically limited by speckles induced by uncorrected aberrations. These aberrations or…

astro-ph.IM2021★ 3 cited

Design of the vacuum high contrast imaging testbed for CDEEP, the Coronagraphic Debris and Exoplanet Exploring Pioneer

Erin R. Maier, Ewan S. Douglas, Daewook Kim +26

The Coronagraphic Debris Exoplanet Exploring Payload (CDEEP) is a Small-Sat mission concept for high contrast imaging of circumstellar disks. CDEEP is designed to observe disks in…

astro-ph.IM2021★ 3 cited

Experimental validation of active control of low-order aberrations with a Zernike sensor through a Lyot coronagraph

Raphaël Pourcelot, Mamadou N'Diaye, Emiel H. Por +11

Future large segmented space telescopes and their coronagraphic instruments are expected to provide the resolution and sensitivity to observe Earth-like planets with a 10^10 contra…