Diffraction-limited imaging of stellar objects using telescopes of low optical quality

JC Dainty - Optics Communications, 1973 - Elsevier
DIFFRACTION-LIMITED IMAGING OF STELLAR OBJECTS USING TELESCOPES OF LOW
OPTICAL QUALITY JC DAINTY 1. Introduction Labeyrie has Page 1 Volume I, number 2 …
被引用次数：96 相关文章 所有 3 个版本
[PDF] harvard.edu

Attainment of diffraction limited resolution in large telescopes by Fourier analysing speckle patterns in star images

A Labeyrie - Astronomy and Astrophysics, Vol. 6, p. 85 (1970), 1970 - adsabs.harvard.edu
Resolution in excess of the limitation set by seeing, and reaching the diffraction value, can
be obtained on star features by laser processing the speckle paftern observed in short …
被引用次数：1818 相关文章 所有 8 个版本
[PDF] harvard.edu

Stellar interferometry methods

A Labeyrie - Annual review of astronomy and astrophysics, 1978 - annualreviews.org
Stellar interferometry may be defined as the art of utilizing interference effects for improving
the angular resolution of stellar observations. Resolution is improved in two ways:(a) …
被引用次数：159 相关文章 所有 6 个版本
[HTML] harvard.edu

[HTML][HTML] Diffraction-limited imaging. II-Optical aperture-synthesis imaging of two binary stars

T Nakajima, SR Kulkarni, PW Gorham… - … Journal (ISSN 0004 …, 1989 - adsabs.harvard.edu
Diffraction-limited imaging. II - Optical aperture-synthesis imaging of two bina ADS Classic is
now deprecated. It will be completely retired in October 2019. This page will automatically …
被引用次数：83 相关文章 所有 6 个版本
[HTML] harvard.edu

[HTML][HTML] Autocorrelation Methods to Obtain Diffraction-Limited Resolution with Large Telescopes

CE KenKnight - Astrophysical Journal, vol. 176, p. L43, 1972 - adsabs.harvard.edu
Autocorrelation Methods to Obtain Diffraction-Limited Resolution with Large Tele ADS Classic is
now deprecated. It will be completely retired in October 2019. This page will automatically …
被引用次数：23 相关文章 所有 4 个版本

Interferometric imaging in optical astronomy

F Roddier - Physics Reports, 1988 - Elsevier
It is learned from elementary textbooks that the angular resolution of a perfect optical
telescope is limited by diffraction to an angle in radians of about A ID, the ratio of the …
被引用次数：190 相关文章 所有 5 个版本
[HTML] aanda.org

[HTML][HTML] Long-baseline optical intensity interferometry-laboratory demonstration of diffraction-limited imaging

D Dravins, T Lagadec, PD Nuñez - Astronomy & Astrophysics, 2015 - aanda.org
Context. A long-held vision has been to realize diffraction-limited optical aperture synthesis
over kilometer baselines. This will enable imaging of stellar surfaces and their environments …
被引用次数：32 相关文章 所有 10 个版本

Computer simulation of a method for object reconstruction from stellar speckle interferometry data

JG Walker - Applied Optics, 1982 - opg.optica.org
A method for reconstructing a diffraction-limited image from data consisting of many short-
exposure turbulence degraded images is described. The results of a computer simulation of …
被引用次数：45 相关文章 所有 8 个版本
[PDF] harvard.edu

The transfer function, signal-to-noise ratio, and limiting magnitude in stellar speckle interferometry

JC Dainty, J Ring - Monthly Notices of the Royal Astronomical …, 1974 - academic.oup.com
Recent theoretical work has shown that atmospheric seeing which would be regarded as
poor for conventional imaging is desirable for attaining diffraction-limited resolution from an …
被引用次数：80 相关文章 所有 4 个版本
[HTML] harvard.edu

[HTML][HTML] Speckle interferometry: diffraction-limited measurements of nine stars with the 200-inch telescope

DY Gezari, A Labeyrie… - Astrophysical Journal, vol …, 1972 - adsabs.harvard.edu
A new method has enabled us to repeat most of the classical Michelson-Pease
measurements of stellar diameters. Stellar images are photographed" coherently" with a …
被引用次数：286 相关文章 所有 5 个版本