activity
20142026
most citedThe Gemini Planet Imager: First Light

714 citations · 5.5k across the 123 of their papers we have counts for

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41 papers · 1 filter

astro-ph.IM2026

Demonstration of simultaneous PIAA- coronagraphy and wavefront sensing using a single metasurface-based focal-plane optic

Dhwanil Patel, Sebastiaan Y. Haffert, Skyler Palatnick +23

Controlling residual wavefront aberrations downstream of an extreme adaptive optics (ExAO) system is a major challenge in high-contrast imaging. These aberrations produce quasi-sta…

astro-ph.IM2026

The Roman Coronagraph Community Participation Program: data reduction pipeline astrometric calibration

Amanda Chavez, Jason Wang, Vanessa P. Bailey +5

The Nancy Grace Roman Space Telescope will be equipped with a Technology Demonstration Coronagraph Instrument that will push the current limits of high contrast imaging for exoplan…

astro-ph.IM2026

The Roman Coronagraph Community Participation Program: calibration strategy for the Mueller matrix using on-sky sources

Toshiyuki Mizuki, Justin Hom, Bertrand Mennesson +14

The Nancy Grace Roman Space Telescope Coronagraph Instrument will provide space-based polarimetric observations of circumstellar disks and exoplanetary systems. Accurate reconstruc…

astro-ph.IM2025

Performance Simulations for Kola: Achieving High-Resolution, Visible-Light AO Correction Over a 1 Arcminute Field

Brianna Peck, Jessica R. Lu, Lianqi Wang +8

We present performance simulations for a proposed visible-light, multi-conjugate adaptive optics system for the 10-meter W. M. Keck I telescope that aims to deliver near diffractio…

astro-ph.IM2025

Habitable World Discovery and Characterization: Coronagraph Concept of Operations and Data Post-Processing

Michael W. McElwain, Dimitri Mawet, Jean-Baptiste Ruffio +11

The discovery and characterization of habitable worlds was the top scientific recommendation of the Astro2020 decadal survey and is a key objective of the Habitable Worlds Observat…

astro-ph.IM2025

Identifying rocky planets and water worlds among sub-Neptune-sized exoplanets with the Habitable Worlds Observatory

Renyu Hu, Michiel Min, Max Millar-Blanchaer +15

Astronomers are debating whether the plentiful "sub-Neptune" exoplanets -- worlds a bit larger than Earth but smaller than Neptune -- are predominantly rocky planets, water-rich "o…

astro-ph.IM2025

PIRATES -- a machine-learning framework for polarized, interferometric image reconstruction

Lucinda Lilley, Barnaby Norris, Peter Tuthill +13

Optical interferometric image reconstruction is a challenging, ill-posed optimization problem which usually relies on heavy regularization for convergence. Conventional algorithms…

astro-ph.IM2025★ 4 cited

Polarization aberrations in next-generation Giant Segmented Mirror Telescopes (GSMTs). II. Influence of segment-to-segment coating variations on high-contrast imaging and polarimetry

Jaren N. Ashcraft, Ramya M. Anche, Sebastiaan Y. Haffert +8

Direct exo-Earth imaging is a key science goal for astronomy in the next decade. This ambitious task imposes a target contrast of ~10^-7 at wavelengths from I to J-band. In our pri…

astro-ph.IM2024★ 6 cited

The Roman coronagraph community participation program: observation planning

Schuyler G. Wolff, Jason Wang, Karl Stapelfeldt +18

The Coronagraphic Instrument onboard the Nancy Grace Roman Space Telescope is an important stepping stone towards the characterization of habitable, rocky exoplanets. In a technolo…

astro-ph.IM2024

Visible-Light High-Contrast Imaging and Polarimetry with SCExAO/VAMPIRES

Miles Lucas, Barnaby Norris, Olivier Guyon +17

We present significant upgrades to the VAMPIRES instrument, a visible-light (600 nm to 800 nm) high-contrast imaging polarimeter integrated within SCExAO on the Subaru telescope. K…

astro-ph.IM2024

The space coronagraph optical bench (SCoOB): 3. Mueller matrix polarimetry of a coronagraphic exit pupil

Jaren N. Ashcraft, Ewan S. Douglas, Ramya M. Anche +4

High-contrast imaging in the next decade aims to image exoplanets at smaller angular separations and deeper contrasts than ever before. A problem that has recently garnered attenti…

astro-ph.IM2024

The Space Coronagraph Optical Bench (SCoOB): 5. End-to-end simulations of polarization aberrations

Ramya M Anche, Kyle J. Van Gorkom, Jaren N. Ashcraft +4

Polarization aberrations originating from the telescope and high-contrast imaging instrument optics introduce polarization-dependent speckles and associated errors in the image pla…

astro-ph.IM2023

Exploring calibration algorithms to maximize the null depth in KPIC's vortex fiber nulling mode

Sofia Hillman, Daniel Echeverri, Maxwell A. Millar-Blanchaer +3

Vortex fiber nulling (VFN) is a new interferometric technique with the potential to unlock the ability to detect and spectroscopically characterize exoplanets at angular separation…

astro-ph.IM2023

The development of HISPEC for Keck and MODHIS for TMT: science cases and predicted sensitivities

Quinn M. Konopacky, Ashley D. Baker, Dimitri Mawet +72

HISPEC is a new, high-resolution near-infrared spectrograph being designed for the W.M. Keck II telescope. By offering single-shot, R=100,000 between 0.98 - 2.5 um, HISPEC will ena…

astro-ph.IM2023★ 12 cited

Vortex Fiber Nulling for Exoplanet Observations: Implementation and First Light

Daniel Echeverri, Jerry Xuan, Nemanja Jovanovic +31

Vortex fiber nulling (VFN) is a single-aperture interferometric technique for detecting and characterizing exoplanets separated from their host star by less than a diffracted beam…

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

Estimation of polarization aberrations and their effect on the coronagraphic performance for future space telescopes

Ramya M Anche, Sebastiaan Y. Haffert, Jaren N Ashcraft +5

A major goal of proposed future space observatories, such as the Habitable World Observatory, is to directly image and characterize Earth-like planets around Sun-like stars to sear…

astro-ph.IM2023★ 19 cited

Polarization aberrations in next-generation giant segmented mirror telescopes (GSMTs) I. Effect on the coronagraphic performance

Ramya M. Anche, Jaren N. Ashcraft, Sebastiaan Y. Haffert +8

Next-generation large segmented mirror telescopes are expected to perform direct imaging and characterization of Earth-like rocky planets, which requires contrast limits of $10^{-7…

astro-ph.IM2023

The JWST Early Release Science Program for Direct Observations of Exoplanetary Systems: Best Practices for Data Collection in Cycle 2 and Beyond

Sasha Hinkley, Beth Biller, Andrew Skemer +35

We present a set of recommended best practices for JWST data collection for members of the community focussed on the direct imaging and spectroscopy of exoplanetary systems. These…

astro-ph.IM2022★ 7 cited

A Decade of Linear and Circular Polarimetry with the POLISH2 Polarimeter

Sloane J. Wiktorowicz, Agnieszka Słowikowska, Larissa A. Nofi +15

The POLISH2 optical polarimeter has been in operation at the Lick Observatory 3-m Shane telescope since 2011, and it was commissioned at the Gemini North 8-m in 2016. This instrume…

astro-ph.IM2021

The Planetary Systems Imager Adaptive Optics System: An Initial Optical Design and Performance Analysis Tools for the PSI-Red AO System

Rebecca Jensen-Clem, Philip M. Hinz, M. A. M. van Kooten +10

The Planetary Systems Imager (PSI) is a proposed instrument for the Thirty Meter Telescope (TMT) that provides an extreme adaptive optics (AO) correction to a multi-wavelength inst…

astro-ph.IM2020★ 12 cited

DiskFM: A Forward Modeling Tool for Disk Analysis with Coronagraphic Instruments

Johan Mazoyer, Pauline Arriaga, Justin Hom +6

Because of bright starlight leakage in coronagraphic raw images, faint astrophysical objects such as exoplanets can only be detected using powerful point spread function (PSF) subt…

astro-ph.IM2020

Detecting and characterizing close-in exoplanets with Vortex Fiber Nulling

Daniel Echeverri, Garreth Ruane, Benjamin Calvin +8

Vortex Fiber Nulling (VFN) is an interferometric method for suppressing starlight to detect and spectroscopically characterize exoplanets. It relies on a vortex phase mask and sing…

astro-ph.IM2020★ 2 cited

HD 165054: an astrometric calibration field for high-contrast imagers in Baade's Window

Meiji M. Nguyen, Robert J. De Rosa, Jason J. Wang +51

We present a study of the HD 165054 astrometric calibration field that has been periodically observed with the Gemini Planet Imager. HD 165054 is a bright star within Baade's Windo…