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20022024
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1k citations · 9.6k across the 241 of their papers we have counts for

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Showing 2018 · astro-ph.IMShow all

23 papers · 2 filters

astro-ph.IM2018★ 17 cited

Laser Guide Star for Large Segmented-Aperture Space Telescopes, Part I: Implications for Terrestrial Exoplanet Detection and Observatory Stability

Ewan S. Douglas, Jared R. Males, James Clark +4

Precision wavefront control on future segmented-aperture space telescopes presents significant challenges, particularly in the context of high-contrast exoplanet direct imaging. We…

astro-ph.IM2018★ 64 cited

The Habitable Exoplanet Observatory (HabEx) Mission Concept Study Interim Report

B. Scott Gaudi, Sara Seager, Bertrand Mennesson +79

For the first time in human history, technologies have matured sufficiently to enable a mission capable of discovering and characterizing habitable planets like Earth orbiting sunl…

astro-ph.IM2018★ 26 cited

SCExAO, an instrument with a dual purpose: perform cutting-edge science and develop new technologies

Julien Lozi, Olivier Guyon, Nemanja Jovanovic +31

The Subaru Coronagraphic Extreme Adaptive Optics (SCExAO) instrument is an extremely modular high-contrast instrument installed on the Subaru telescope in Hawaii. SCExAO has a dual…

astro-ph.IM2018★ 19 cited

Characterizing Vibrations at the Subaru Telescope for the Subaru Coronagraphic Extreme Adaptive Optics instrument

Julien Lozi, Olivier Guyon, Nemanja Jovanovic +6

Vibrations are a key source of image degradation in ground-based instrumentation, especially for high-contrast imaging instruments. Vibrations reduce the quality of the correction…

astro-ph.IM2018

The Planetary Systems Imager: 2-5 Micron Channel

Andrew J. Skemer, Deno Stelter, Dimitri Mawet +15

We summarize the red channel (2-5 micron) of the Planetary Systems Imager (PSI), a proposed second-generation instrument for the TMT. Cold exoplanets emit the majority of their lig…

astro-ph.IM2018

SHARK-NIR, the coronagraphic camera for LBT, moving toward construction

Jacopo Farinato, Francesca Bacciotti, Carlo Baffa +37

SHARK-NIR is one of the two coronagraphic instruments proposed for the Large Binocular Telescope. Together with SHARK-VIS (performing coronagraphic imaging in the visible domain),…

astro-ph.IM2018

Review of high-contrast imaging systems for current and future ground-based and space-based telescopes III. Technology opportunities and pathways

Frans Snik, Olivier Absil, Pierre Baudoz +30

The Optimal Optical CoronagraphWorkshop at the Lorentz Center in September 2017 in Leiden, the Netherlands gathered a diverse group of 25 researchers working on exoplanet instrumen…

astro-ph.IM2018★ 8 cited

Review of high-contrast imaging systems for current and future ground-based and space-based telescopes II. Common path wavefront sensing/control and Coherent Differential Imaging

Nemanja Jovanovic, Olivier Absil, Pierre Baudoz +28

The Optimal Optical Coronagraph (OOC) Workshop held at the Lorentz Center in September 2017 in Leiden, the Netherlands, gathered a diverse group of 25 researchers working on exopla…

astro-ph.IM2018★ 18 cited

Review of high-contrast imaging systems for current and future ground- and space-based telescopes I. Coronagraph design methods and optical performance metrics

G. Ruane, A. Riggs, J. Mazoyer +29

The Optimal Optical Coronagraph (OOC) Workshop at the Lorentz Center in September 2017 in Leiden, the Netherlands gathered a diverse group of 25 researchers working on exoplanet in…

astro-ph.IM2018

Modeling coronagraphic extreme wavefront control systems for high contrast imaging in ground and space telescope missions

Jennifer Lumbres, Jared Males, Ewan Douglas +17

The challenges of high contrast imaging (HCI) for detecting exoplanets for both ground and space applications can be met with extreme adaptive optics (ExAO), a high-order adaptive…

astro-ph.IM2018

Focal plane wavefront sensing and control strategies for high-contrast imaging on the MagAO-X instrument

Kelsey Miller, Jared R. Males, Olivier Guyon +14

The Magellan extreme adaptive optics (MagAO-X) instrument is a new extreme adaptive optics (ExAO) system designed for operation in the visible to near-IR which will deliver high co…

astro-ph.IM2018

Phase-induced amplitude apodization complex mask coronagraph tolerancing and analysis

Justin M. Knight, Olivier Guyon, Julien Lozi +2

Phase-Induced Amplitude Apodization Complex Mask Coronagraphs (PIAACMC) offer high-contrast performance at a small inner-working angle ( 1 /D) with high planet throughp…

astro-ph.IM2018★ 5 cited

Characterization of deformable mirrors for the MagAO-X project

Kyle Van Gorkom, Kelsey L. Miller, Jared R. Males +4

The MagAO-X instrument is an upgrade of the Magellan AO system that will introduce extreme adaptive optics capabilities for high-contrast imaging at visible and near-infrared wavel…

astro-ph.IM2018★ 4 cited

Real-time estimation and correction of quasi-static aberrations in ground-based high contrast imaging systems with high frame-rates

Alexander T. Rodack, Jared R. Males, Olivier Guyon +3

The success of ground-based, high contrast imaging for the detection of exoplanets in part depends on the ability to differentiate between quasi-static speckles caused by aberratio…

astro-ph.IM2018

Design of the MagAO-X Pyramid Wavefront Sensor

Lauren H. Schatz, Jared R. Males, Laird M. Close +11

Adaptive optics systems correct atmospheric turbulence in real time. Most adaptive optics systems used routinely correct in the near infrared, at wavelengths greater than 1 micron.…

astro-ph.IM2018

MagAO-X: project status and first laboratory results

Jared R. Males, Laird M. Close, Kelsey Miller +32

MagAO-X is an entirely new "extreme" adaptive optics system for the Magellan Clay 6.5 m telescope, funded by the NSF MRI program starting in Sep 2016. The key science goal of MagAO…

astro-ph.IM2018

The Robo-AO-2 facility for rapid visible/near-infrared AO imaging and the demonstration of hybrid techniques

Christoph Baranec, Mark Chun, Donald Hall +23

We are building a next-generation laser adaptive optics system, Robo-AO-2, for the UH 2.2-m telescope that will deliver robotic, diffraction-limited observations at visible and nea…

astro-ph.IM2018★ 25 cited

Overview of the SAPHIRA Detector for AO Applications

Sean B. Goebel, Donald N. B. Hall, Olivier Guyon +2

We discuss some of the unique details of the operation and behavior of Leonardo SAPHIRA detectors, particularly in relation to their usage for adaptive optics wavefront sensing. SA…

astro-ph.IM2018

TDEM final report: Enhanced direct imaging exoplanet detection with astrometry mass determination

Eduardo Bendek, Ruslan Belikov, Olivier Guyon +6

This Final Report (FR) presents the results of the Enhanced direct imaging exoplanet detection with astrometry mass determination project, which was executed in support of NASA's E…

astro-ph.IM2018★ 1 cited

Project Blue: Visible Light Imaging Search for Terrestrial-class Exoplanets in the Habitable Zones of Alpha Centauri A and B

Jon Morse, Eduardo Bendek, Nathalie Cabrol +9

Project Blue is designed to deliver a small coronagraphic space telescope mission to low-Earth orbit capable of detecting an Earth-like planet in the habitable zones of the Sun-lik…

astro-ph.IM2018

The value of astrometry for exoplanet science

Eduardo Bendek, Mark Marley, Michael Shao +3

Exoplanets mass measurements will be a critical next step to assess the habitability of Earth-like planets: a key aspect of the 2020 vision in the previous decadal survey and also…

astro-ph.IM2018★ 1 cited

Precision Space Astrometry as a Tool to Find Earth-like Exoplanets

Michael Shao, Slava G. Turyshev, Eduardo Bendek +6

Because of the recent technological advances, the key technologies needed for precision space optical astrometry are now in hand. The Microarcsecond Astrometry Probe (MAP) mission…

astro-ph.IM2018★ 19 cited

Laboratory and On-Sky Validation of the Shaped Pupil Coronagraph's Sensitivity to Low-Order Aberrations With Active Wavefront Control

Thayne Currie, N. Jeremy Kasdin, Tyler Groff +10

We present early laboratory simulations and extensive on-sky tests validating of the performance of a shaped pupil coronagraph (SPC) behind an extreme-AO corrected beam of the Suba…