Search Results - "Neichel, B"
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1
Blind deconvolution in astronomy with adaptive optics: the parametric marginal approach
Published in Monthly notices of the Royal Astronomical Society (21-08-2020)“…ABSTRACT One of the major limitations of using adaptive optics (AO) to correct image post-processing is the lack of knowledge about the system’s point spread…”
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Limitations imposed by optical turbulence profile structure and evolution on tomographic reconstruction for the ELT
Published in Monthly notices of the Royal Astronomical Society (11-05-2020)“…ABSTRACT The performance of tomographic adaptive optics (AO) systems is intrinsically linked to the vertical profile of optical turbulence. First, a sufficient…”
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3
PRIME: PSF Reconstruction and Identification for Multiple-source characterization Enhancement – application to Keck NIRC2 imager
Published in Monthly notices of the Royal Astronomical Society (21-08-2019)“…ABSTRACT In order to enhance the scientific exploitation of adaptive optics (AO)-assisted observations, we investigate a novel hybrid concept to improve the…”
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4
Optimal correction of distortion for high-angular-resolution images: Application to GeMS data
Published in Monthly notices of the Royal Astronomical Society (01-01-2018)“…Whether ground based or space based, any optical instrument suffers from some amount of optical geometric distortion. Recently, the diffraction-limited image…”
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5
Pushing point-spread function reconstruction to the next level: application to SPHERE/ZIMPOL
Published in Monthly notices of the Royal Astronomical Society (01-05-2020)“…ABSTRACT Point-spread function (PSF) reconstruction (PSF-R) is a well-established technique to determine the PSF reliably and accurately from adaptive optics…”
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Towards an automatic wind speed and direction profiler for Wide Field adaptive optics systems
Published in Monthly notices of the Royal Astronomical Society (01-05-2018)“…Wide Field Adaptive Optics (WFAO) systems are among the most sophisticated AO systems available today on large telescopes. The knowledge of the vertical…”
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7
A new calibration strategy for adaptive telescopes with pyramid WFS
Published in Monthly notices of the Royal Astronomical Society (01-12-2018)Get full text
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8
SPRINT, system parameters recurrent invasive tracking: a fast and least-cost online calibration strategy for adaptive optics
Published in Monthly notices of the Royal Astronomical Society (01-07-2021)“…ABSTRACT Future large adaptive telescopes will trigger new constraints for the calibration of adaptive optics (AO) systems equipped with pre-focal deformable…”
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Off-axis point spread function characterization in laser guide star adaptive optics systems
Published in Monthly notices of the Royal Astronomical Society (21-08-2018)“…ABSTRACT Adaptive optics (AO) restore the angular resolution of ground-based telescopes, but at the cost of delivering a time- and space-varying point spread…”
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10
Identifying optical turbulence profiles for realistic tomographic error in adaptive optics
Published in Monthly notices of the Royal Astronomical Society (01-09-2019)“…ABSTRACT For extremely large telescopes, adaptive optics will be required to correct the Earth’s turbulent atmosphere. The performance of tomographic adaptive…”
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The Proper Motion of Pyxis: The First Use of Adaptive Optics in Tandem with HST on a Faint Halo Object
Published in The Astrophysical journal (01-05-2017)“…We present a proper motion measurement for the halo globular cluster Pyxis, using Hubble Space Telescope/ACS data as the first epoch and GeMS/GSAOI Adaptive…”
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12
Characterization of the sodium layer at Cerro Pachón, and impact on laser guide star performance
Published in Monthly notices of the Royal Astronomical Society (11-03-2013)“…Detailed knowledge of the mesospheric sodium layer characteristics is crucial to estimate and optimize the performance of laser guide star (LGS) assisted…”
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13
Online estimation of the wavefront outer scale profile from adaptive optics telemetry
Published in Monthly notices of the Royal Astronomical Society (01-02-2017)“…We describe an online method to estimate the wavefront outer scale profile, L0(h), for very large and future extremely large telescopes. The stratified…”
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14
Simulating the detection and classification of high-redshift supernovae with HARMONI on the ELT
Published in Monthly notices of the Royal Astronomical Society (11-08-2018)“…We present detailed simulations of integral field spectroscopic observations of a supernova in a host galaxy at z ∼ 3, as observed by the HARMONI spectrograph…”
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15
Gemini multiconjugate adaptive optics system review - I. Design, trade-offs and integration
Published in Monthly notices of the Royal Astronomical Society (21-01-2014)Get full text
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16
Simulating the physics and mass assembly of distant galaxies out to z∼ 6 with the E-ELT
Published in Monthly notices of the Royal Astronomical Society (2010)“…One of the main scientific goals of the future European Extremely Large Telescope (E-ELT) will be to understand the mass assembly process in galaxies as a…”
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17
Coupling MOAO with integral field spectroscopy: specifications for the VLT and the E-ELT
Published in Monthly notices of the Royal Astronomical Society (01-11-2008)“…Elucidating the processes that governed the assembly and evolution of galaxies over cosmic time is one of the main objectives of all of the proposed Extremely…”
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18
Modeling and Estimation of Adaptive Optics-Corrected long-exposure Point Spread Function Using Gaussian Sum Approximation
Published in Monthly notices of the Royal Astronomical Society (15-11-2024)“…Abstract Adaptive optics (AO) enhances astronomical images by correcting perturbations in the optical system, resulting in complex point spread function (PSF)…”
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An upper limit to the sodium layer longitudinal and transversal altitude structure function from MCAO data
Published in Monthly notices of the Royal Astronomical Society. Letters (15-05-2013)“…The Gemini Multi-Conjugate Adaptive Optics System is the first sodium-based Multi-Laser Guide Star (LGS) Adaptive Optics system used for astronomy. It uses…”
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Current status of PAPYRUS : the pyramid based adaptive optics system at LAM/OHP
Published 19-10-2021“…Proc. SPIE 11876, Optical Instrument Science, Technology, and Applications II, 118760H (24 September 2021); The Provence Adaptive optics Pyramid Run System…”
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