Aperture Masking Imaging
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Description
Aperture-mask interferometry has a long history in the speckle regime � in principle equalling the performance of speckle interferometry in the low-flux, zero read-noise regime and offering superior calibration in the bright regime. Since adaptive optics has become commonplace on large telescopes, the key advantage of aperture-mask interferometry is in calibration, particularly of low spatial-frequency phase aberrations that cause quasi-static speckles. I will describe the principles of...[Show more]
Collections | ANU Research Publications |
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Date published: | 2016 |
Type: | Journal article |
URI: | http://hdl.handle.net/1885/154846 |
Source: | Astrophysics and Space Science Library |
Book Title: | Astronomy at High Angular Resolution Astronomy at High Angular Resolution |
DOI: | 10.1007/978-3-319-39739-9 |
Access Rights: | Open Access |
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File | Description | Size | Format | Image |
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Aperture masking imaging.pdf | 462.53 kB | Adobe PDF |
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