An improved distance and mass estimate for Sgr A* from a multistar orbit analysis

A Boehle, AM Ghez, R Schödel, L Meyer… - The Astrophysical …, 2016 - iopscience.iop.org
We present new, more precise measurements of the mass and distance of our Galaxy's
central supermassive black hole, Sgr A*. These results stem from a new analysis that more …

[書籍][B] Principles of adaptive optics

RK Tyson, BW Frazier - 2022 - taylorfrancis.com
Principles of Adaptive Optics describes the foundations, principles, and applications of
adaptive optics (AO) and its enabling technologies. This leading textbook addresses the …

[書籍][B] Imaging through turbulence

MC Roggemann, BM Welsh - 2018 - taylorfrancis.com
Learn how to overcome resolution limitations caused by atmospheric turbulence in Imaging
Through Turbulence. This hands-on book thoroughly discusses the nature of turbulence …

Physics-driven turbulence image restoration with stochastic refinement

A Jaiswal, X Zhang, SH Chan… - Proceedings of the IEEE …, 2023 - openaccess.thecvf.com
Image distortion by atmospheric turbulence is a stochastic degradation, which is a critical
problem in long-range optical imaging systems. A number of research has been conducted …

Joint estimation of object and aberrations by using phase diversity

RG Paxman, TJ Schulz, JR Fienup - JOSA A, 1992 - opg.optica.org
The joint estimation of an object and the aberrations of an incoherent imaging system from
multiple images incorporating phase diversity is investigated. Maximum-likelihood …

Multiframe blind deconvolution of astronomical images

TJ Schulz - JOSA A, 1993 - opg.optica.org
Maximum-likelihood estimation techniques are presented for the problem of forming object
estimates from turbulence-degraded images when the point-spread functions are unknown …

Wave-front temporal spectra in high-resolution imaging through turbulence

JM Conan, G Rousset, PY Madec - JOSA A, 1995 - opg.optica.org
A general formulation is given for the derivation of theoretical temporal power spectra of
quantities related to turbulent wave-front phase. These temporal power spectra and their …

The shortest-known–period star orbiting our galaxy's supermassive black hole

L Meyer, AM Ghez, R Schödel, S Yelda, A Boehle… - Science, 2012 - science.org
Stars with short orbital periods at the center of our Galaxy offer a powerful probe of a
supermassive black hole. Over the past 17 years, the WM Keck Observatory has been used …

Wave-front reconstruction using a Shack–Hartmann sensor

RG Lane, M Tallon - Applied optics, 1992 - opg.optica.org
An analysis of the problem of wave-front reconstruction from Shack–Hartmann
measurements is presented. The wave-front aberration is assumed to result from passage of …

[書籍][B] Microoptics

S Sinzinger, J Jahns - 2006 - books.google.com
In dieser zweiten Auflage ergänzen Stefan Sinzinger und Jürgen Jahns ihr modernes Lehr-
und Nachschlagebuch, das Grundlagen und Anwendungen der Mikrooptik kompetent und …