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 …
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 …
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 …
Through Turbulence. This hands-on book thoroughly discusses the nature of turbulence …
Physics-driven turbulence image restoration with stochastic refinement
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 …
problem in long-range optical imaging systems. A number of research has been conducted …
Joint estimation of object and aberrations by using phase diversity
The joint estimation of an object and the aberrations of an incoherent imaging system from
multiple images incorporating phase diversity is investigated. Maximum-likelihood …
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 …
estimates from turbulence-degraded images when the point-spread functions are unknown …
Wave-front temporal spectra in high-resolution imaging through turbulence
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 …
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 …
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 …
measurements is presented. The wave-front aberration is assumed to result from passage of …