activity
20182023
most citedDisentangling the planet from the star in late type M dwarfs: A case study of TRAPPIST-1g

100 citations · 141 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.EP2023★ 38 cited

Chasing rainbows and ocean glints: Inner working angle constraints for the Habitable Worlds Observatory

Sophia R. Vaughan, Timothy D. Gebhard, Kimberly Bott +41

NASA is engaged in planning for a Habitable Worlds Observatory (HabWorlds), a coronagraphic space mission to detect rocky planets in habitable zones and establish their habitabilit…

astro-ph.EP2022

Battle of the Predictive Wavefront Controls: Comparing Data and Model-Driven Predictive Control for High Contrast Imaging

J. Fowler, Maaike A. M. Van Kooten, Rebecca Jensen-Clem

Ground-based high contrast exoplanet imaging requires state-of-the-art adaptive optics (AO) systems in order to detect extremely faint planets next to their brighter host stars. Fo…

astro-ph.IM2022

Predictive wavefront control on Keck II adaptive optics bench: on-sky coronagraphic results

Maaike A. M. van Kooten, Rebecca Jensen-Clem Sylvain Cetre, Sam Ragland +3

The behavior of an adaptive optics (AO) system for ground-based high contrast imaging (HCI) dictates the achievable contrast of the instrument. In conditions where the coherence ti…

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

Wavefront Sensing and Control with the Many Headed Hydra Modal Basis

J. Fowler, R. Deno Stelter

The future of space and ground based telescopes is intimately tied to technology and algorithm development surrounding wavefront sensing and control. Only with cutting edge develop…

astro-ph.IM2021

The Santa Cruz Extreme AO Lab (SEAL): Design and First Light

Rebecca Jensen-Clem, Daren Dillon, Benjamin Gerard +9

The Santa Cruz Extreme AO Lab (SEAL) is a new visible-wavelength testbed designed to advance the state of the art in wavefront control for high contrast imaging on large, segmented…

astro-ph.IM2021

Status of predictive wavefront control on Keck II adaptive optics bench: on-sky coronagraphic results

Maaike A. M. van Kooten, Rebecca Jensen-Clem, Sylvain Cetre +4

The behavior of an adaptive optics (AO) system for ground-based high contrast imaging (HCI) dictates the achievable contrast of the instrument. In conditions where the coherence ti…

astro-ph.IM2020

Estimating low-order aberrations through a Lyot coronagraph with a Zernike wavefront sensor for exoplanet imaging

Raphaël Pourcelot, Mamadou N'Diaye, Greg Brady +13

Imaging exo-Earths is an exciting but challenging task because of the 10^-10 contrast ratio between these planets and their host star at separations narrower than 100 mas. Large se…

astro-ph.IM2020★ 3 cited

Predicting contrast sensitivity to segmented aperture misalignment modes for the HiCAT testbed

Iva Laginja, Remi Soummer, Laurent M. Mugnier +10

This paper presents the setup for empirical validations of the Pair-based Analytical model for Segmented Telescope Imaging from Space (PASTIS) tolerancing model for segmented coron…

astro-ph.EP2018★ 100 cited

Disentangling the planet from the star in late type M dwarfs: A case study of TRAPPIST-1g

Hannah R. Wakeford, Nikole K. Lewis, Julia Fowler +10

The atmospheres of late M stars represent a significant challenge in the characterization of any transiting exoplanets due to the presence of strong molecular features in the stell…