activity
20152026
most citedUsing the Multi-Object Adaptive Optics demonstrator RAVEN to observe metal-poor stars in and towards the Galactic Centre

24 citations · 120 across the 14 of their papers we have counts for

collaborators

15 papers

astro-ph.IM2026

AO3k + SCExAO: on-sky wavefront quality and demonstration of novel WFS techniques with the double XAO system

Julien Lozi, Kyohoon Ahn, Vincent Deo +5

The Subaru Coronagraphic Extreme Adaptive Optics (SCExAO) system, fed by its upstream 3000-actuator "woofer" (AO3k), serves both as a platform for high contrast imaging (HCI) techn…

astro-ph.EP2026

SCExAO/CHARIS High-Contrast Pre-Launch Vetting of Roman Coronagraph Technology Demonstration PSF Reference Stars

Thayne Currie, Jie Li, Mona El Morsy +9

We present deep, SCExAO/CHARIS high-contrast integral field spectroscopy and archival imaging of four candidate Roman Coronagraph PSF reference stars within/near the Roman Continuo…

astro-ph.EP2026

Technology and Science Advancing Observations with Roman Coronagraph Informed by Ground-Based High-Contrast Imaging

Mona El Morsy, Thayne Currie, Brianna Lacy +10

The Roman Coronagraph technology demonstration focuses on achieving 10 contrasts within the instrument's dark hole and our ability to detect and characterize properties…

astro-ph.IM2024

AO3k at Subaru: First on-sky results of the facility extreme-AO

Julien Lozi, Kyohoon Ahn, Hannah Blue +12

The facility adaptive optics of the Subaru Telescope AO188 recently received some long-awaited upgrades: a new 3224-actuator deformable mirror (DM) from ALPAO (hence the name chang…

astro-ph.IM2023

SHARPEST: The atmospheric turbulence profiling experiment using Shack-Hartmann sensor at the Subaru telescope

Hajime Ogane, Yoshito Ono, Yosuke Minowa +5

Atmospheric turbulence profile plays an important role in designing and operating adaptive optics (AO) systems with multiple laser guide stars. To obtain representative free atmosp…

astro-ph.IM2022★ 16 cited

AO3000 at Subaru: Combining for the first time a NIR WFS using First Light's C-RED ONE and ALPAO's 64x64 DM

Julien Lozi, Kyohoon Ahn, Christophe Clergeon +7

After 16 years of on-sky operation, Subaru Telescope's facility adaptive optics AO188 is getting several major upgrades to become the extreme-AO AO3000 (3000 actuators in the pupil…

astro-ph.IM2022

High Contrast and High Angular Imaging at Subaru Telescope

Olivier Guyon, Kyohoon Ahn, Masayuki Akiyama +10

Adaptive Optics projects at Subaru Telescope span a wide field of capabilities ranging from ground-layer adaptive optics (GLAO) providing partial correction over a 20 arcmin FOV to…

astro-ph.IM2021★ 17 cited

Atmospheric turbulence profiling with multi-aperture scintillation of a Shack-Hartmann sensor

Hajime Ogane, Masayuki Akiyama, Shin Oya +1

Adaptive optics (AO) systems using tomographic estimation of three-dimensional structure of atmospheric turbulence requires vertical atmospheric turbulence profile, which describes…

astro-ph.IM2018★ 7 cited

Fast Iterative Tomographic Wave-front Estimation with Recursive Toeplitz Reconstructor Structure for Large Scale Systems

Yoshito H. Ono, Carlos Correia, Rodolphe Conan +3

Tomographic wave-front reconstruction is the main computational bottleneck to realize real-time correction for turbulence-induced wave-front aberrations in future laser-assisted to…

astro-ph.IM2016★ 24 cited

Using the Multi-Object Adaptive Optics demonstrator RAVEN to observe metal-poor stars in and towards the Galactic Centre

Masen Lamb, Kim Venn, David Andersen +16

The chemical abundances for five metal-poor stars in and towards the Galactic bulge have been determined from H-band infrared spectroscopy taken with the RAVEN multi-object adaptiv…

astro-ph.GA2016★ 8 cited

Cluster Glimpses with Raven: AO Corrected Near and Mid-Infrared Images of Glimpse C01 and Glimpse C02

T. J. Davidge, D. R. Andersen, O. Lardiere +9

We discuss images of the star clusters GLIMPSE C01 (GC01) and GLIMPSE C02 (GC02) that were recorded with the Subaru IRCS. Distortions in the wavefront were corrected with the RAVEN…

astro-ph.IM2016★ 3 cited

William Herschel Telescope site characterization using the MOAO pathfinder CANARY on-sky data

O. A. Martin, C. M. Correia, E. Gendron +8

Canary is the Multi-Object Adaptive Optics (MOAO) pathfinder for the future MOAO-assisted Integral-Field Units (IFU) proposed for Extremely Large Telescopes (ELT). The MOAO concept…

astro-ph.IM2016★ 18 cited

Statistics of Turbulence Parameters at Maunakea using multiple wave-front sensor data of RAVEN

Yoshito H. Ono, Carlos M. Correia, Dave R. Andersen +5

Prior statistical knowledge of the atmospheric turbulence is essential for designing, optimizing and evaluating tomographic adaptive optics systems. We present the statistics of th…

astro-ph.IM2016★ 18 cited

Multi time-step wave-front reconstruction for tomographic Adaptive-Optics systems

Yoshito H. Ono, Masayuki Akiyama, Shin Oya +5

In tomographic adaptive-optics (AO) systems, errors due to tomographic wave-front reconstruction limit the performance and angular size of the scientific field of view (FoV), where…

astro-ph.GA2015★ 9 cited

Raven and the Center of Maffei 1: Multi-Object Adaptive Optics Observations of the Center of a Nearby Elliptical Galaxy and the Detection of an Intermediate Age Population

T. J. Davidge, D. R. Andersen, O. Lardiere +5

Near-infrared (NIR) spectra that have an angular resolution of ~ 0.15 arcsec are used to examine the stellar content of the central regions of the nearby elliptical galaxy Maffei 1…