Results 1 to 10 of about 44,772 (96)
Which isoplanatic patch size for high angular resolution techniques? [PDF]
The isoplanatic patch size is of interest to reach a high performance with an Adaptive Optics system, since the reference star for its calibration should be located in the same isoplanatic domain than the science source. Different techniques and methods have been developed leading to estimations of the isoplanatic patch but all are model-dependent.
Ziad, Aziz +5 more
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On the isoplanatic patch size in High Angular Resolution Techniques [PDF]
To reach a high performance with an adaptive optics system, we need a calibration using a reference source. This latter should be located in the same isoplanatic domain as the science source. Different techniques and methods have been developed leading to estimations of the isoplanatic patch but all are model-dependent. We developed a new technique for
Ziad, A. +3 more
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Formation and evolution of planetary systems: the impact of high-angular resolution optical techniques [PDF]
The direct images of giant extrasolar planets recently obtained around several main sequence stars represent a major step in the study of planetary systems. These high-dynamic range images are among the most striking results obtained by the current generation of high angular resolution instruments, which will be superseded by a new generation of ...
Absil, Olivier, Mawet, Dimitri
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High-angular-resolution stellar imaging with occultations from the Cassini spacecraft – I. Observational technique [PDF]
9 pages, 6 ...
Stewart, Paul N. +4 more
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The wide-field imaging interferometry testbed: enabling techniques for high angular resolution astronomy [PDF]
The Wide-Field Imaging Interferometry Testbed (WIIT) was designed to develop techniques for wide-field of view imaging interferometry, using "double-Fourier" methods. These techniques will be important for a wide range of future space-based interferometry missions.
S. A. Rinehart +10 more
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High-angular resolution electron diffraction-based techniques aim at measuring relative lattice rotations and elastic strains with an accuracy about 1.10-4 (
Ernould, C. +4 more
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Sin embargo esas estructuras han sido elusivas para los objetos más masivos. En este capítulo se presenta el estudio del objeto masivo: NGC 3603 IRS 9A con la cámara infrarroja de alta resolución angular NACO del Very Large Telescope (VLT). Dichas observaciones se realizaron en el modo interferométrico de NACO, a través de la técnica conocida como ...
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Fourier ptychographic coherence scanning interferometry for 3D morphology of high aspect ratio and composite micro-trenches. [PDF]
Li Y +5 more
europepmc +1 more source
A review of light-field imaging in biomedical sciences. [PDF]
Zhao R +5 more
europepmc +1 more source

