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- Dirk Schmidt
- editor
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- Laura Schreiber
- editor
書誌事項
- 公開日
- 2018-07-10
- DOI
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- 10.1117/12.2312992
- 10.48550/arxiv.1807.04315
- 公開者
- SPIE
説明
MagAO-X is an entirely new "extreme" adaptive optics system for the Magellan Clay 6.5 m telescope, funded by the NSF MRI program starting in Sep 2016. The key science goal of MagAO-X is high-contrast imaging of accreting protoplanets at H$��$. With 2040 actuators operating at up to 3630 Hz, MagAO-X will deliver high Strehls (>70%), high resolution (19 mas), and high contrast ($< 1\times10^{-4}$) at H$��$ (656 nm). We present an overview of the MagAO-X system, review the system design, and discuss the current project status.
Presented at SPIE Astronomical Telescopes and Instrumentation 2018
収録刊行物
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- Adaptive Optics Systems VI
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Adaptive Optics Systems VI 10703 9-, 2018-07-10
SPIE
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キーワード
- Earth and Planetary Astrophysics (astro-ph.EP)
- high contrast imaging
- FOS: Physical sciences
- coronagraphs
- adaptive optics
- 620
- wavefront control
- exoplanets
- wavefront sensing
- Astrophysics - Instrumentation and Methods for Astrophysics
- Instrumentation and Methods for Astrophysics (astro-ph.IM)
- Astrophysics - Earth and Planetary Astrophysics
詳細情報 詳細情報について
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- CRID
- 1361137043522866560
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- データソース種別
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- Crossref
- OpenAIRE