2006
DOI: 10.1117/1.2354160
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Reduction of the diffraction pattern in segmented apertures

Abstract: New discoveries in astronomy require the use of ever larger telescopes. These telescopes require segmented apertures, since current technology does not provide for the fabrication of monolithic mirrors with diameters much larger than 8 m. As a result, the point spread function ͑PSF͒ of the system presents a diffraction pattern characteristic of the segmentation geometry, and this complicates the task of detecting faint structures with high spatial resolution. In this work, we investigate the use of amplitude f… Show more

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Cited by 3 publications
(2 citation statements)
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“…In other applications, axial resolution is improved [15,22,23]. There are applications where 3D superresolution is expected [13,14,24], or where the depth of focus must be increased [25], or even a diffraction pattern must be modified [26]. Such a great variety of performances can be obtained with annular binary filters.…”
Section: Introductionmentioning
confidence: 99%
“…In other applications, axial resolution is improved [15,22,23]. There are applications where 3D superresolution is expected [13,14,24], or where the depth of focus must be increased [25], or even a diffraction pattern must be modified [26]. Such a great variety of performances can be obtained with annular binary filters.…”
Section: Introductionmentioning
confidence: 99%
“…The smaller segmented mirror could then be combined to form the large mirror. Many work have been done concerning large mirror segmentation and hexagons configurations [2][3][4][5][6][7][8]. The objective of this paper is to examine the effect of varying the number of hexagons that to be fill the telescope aperture on the quality of optical telescope.…”
Section: Introductionmentioning
confidence: 99%