Optimal Asymmetric Apodizations and Shaped Pupils for Planet Finding Coronagraphy
arXiv:astro-ph/0404388 · doi:10.1364/AO.44.001117
Abstract
The realization that direct imaging of extrasolar planets could be technologically feasible within the next decade or so has inspired a great deal of recent research into high-contrast imaging. We ourselves have contributed several design ideas, all of which can be described as shaped pupil coronagraphs. In this paper, we offer a complete and unified survey of asymmetric shaped pupils designs, some of which have been published in our previous papers. We also introduce a promising new design, which we call barcode masks. These masks achieve the required contrast with a fairly large discovery zone and throughput but most importantly they are perhaps the easiest to manufacture and might therefore stand up best to a refined analysis based on vector propogation techniques.
17 pages, 11 figures, submitted to Applied Optics
References in corpus (5)
Cited by in corpus (11)
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- Linear and Bayesian Planet Detection Algorithms for the Terrestrial Planet Finder
- The SPICA coronagraphic instrument (SCI) for the study of exoplanets
- Experimental demonstration of binary shaped pupil mask coronagraphs for telescopes with obscured pupils
- Fast Fourier Optimization: Sparsity Matters
- SPICA infrared coronagraph for the direct observation of exo-planets
- A Binary Shaped Mask Coronagraph for a Segmented Pupil
- High-Contrast Coronagraphy
- Comparative study of manufacturing techniques for coronagraphic binary pupil masks: masks on substrates and free-standing masks
- Coronagraphic demonstration experiment using aluminum mirrors for space infrared astronomical observations