Modeling coronagraphic extreme wavefront control systems for high contrast imaging in ground and space telescope missions
© 2018 SPIE. The challenges of high contrast imaging (HCI) for detecting exoplanets for both ground and space applications can be met with extreme adaptive optics (ExAO), a high-order adaptive optics system that performs wavefront sensing (WFS) and correction at high speed. We describe 2 ExAO optic...
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格式: | Article |
語言: | English |
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SPIE
2021
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在線閱讀: | https://hdl.handle.net/1721.1/137937 |
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author | Lumbres, Jennifer Males, Jared R. Douglas, Ewan S. Close, Laird M. Cahoy, Kerri L. Carlton, Ashley K. Clark, James Doelman, David S. Feinberg, Lee D. Guyon, Olivier Knight, Justin Marlow, Weston Miller, Kelsey L. Morzinski, Katie M. Por, Emiel H. Rodack, Alexander T. Schatz, Lauren Snik, Frans Van Gorkom, Kyle Wilby, Michael J. |
author2 | Massachusetts Institute of Technology. Department of Aeronautics and Astronautics |
author_facet | Massachusetts Institute of Technology. Department of Aeronautics and Astronautics Lumbres, Jennifer Males, Jared R. Douglas, Ewan S. Close, Laird M. Cahoy, Kerri L. Carlton, Ashley K. Clark, James Doelman, David S. Feinberg, Lee D. Guyon, Olivier Knight, Justin Marlow, Weston Miller, Kelsey L. Morzinski, Katie M. Por, Emiel H. Rodack, Alexander T. Schatz, Lauren Snik, Frans Van Gorkom, Kyle Wilby, Michael J. |
author_sort | Lumbres, Jennifer |
collection | MIT |
description | © 2018 SPIE. The challenges of high contrast imaging (HCI) for detecting exoplanets for both ground and space applications can be met with extreme adaptive optics (ExAO), a high-order adaptive optics system that performs wavefront sensing (WFS) and correction at high speed. We describe 2 ExAO optical system designs, one each for ground- based telescopes and space-based missions, and examine them using the angular spectrum Fresnel propagation module within the Physical Optics Propagation in Python (POPPY) package. We present an end-to-end (E2E) simulation of the MagAO-X instrument, an ExAO system capable of delivering 6x10 -5 visible-light raw contrast for static, noncommon path aberrations without atmosphere. We present an E2E simulation of a laser guidestar (LGS) companion spacecraft testbed demonstration, which uses a remote beacon to increase the signal available for WFS and control of the primary aperture segments of a future large space telescope, providing of order 10 factor improvement for relaxing observatory stability requirements. |
first_indexed | 2024-09-23T11:08:48Z |
format | Article |
id | mit-1721.1/137937 |
institution | Massachusetts Institute of Technology |
language | English |
last_indexed | 2024-09-23T11:08:48Z |
publishDate | 2021 |
publisher | SPIE |
record_format | dspace |
spelling | mit-1721.1/1379372023-04-14T19:55:41Z Modeling coronagraphic extreme wavefront control systems for high contrast imaging in ground and space telescope missions Lumbres, Jennifer Males, Jared R. Douglas, Ewan S. Close, Laird M. Cahoy, Kerri L. Carlton, Ashley K. Clark, James Doelman, David S. Feinberg, Lee D. Guyon, Olivier Knight, Justin Marlow, Weston Miller, Kelsey L. Morzinski, Katie M. Por, Emiel H. Rodack, Alexander T. Schatz, Lauren Snik, Frans Van Gorkom, Kyle Wilby, Michael J. Massachusetts Institute of Technology. Department of Aeronautics and Astronautics © 2018 SPIE. The challenges of high contrast imaging (HCI) for detecting exoplanets for both ground and space applications can be met with extreme adaptive optics (ExAO), a high-order adaptive optics system that performs wavefront sensing (WFS) and correction at high speed. We describe 2 ExAO optical system designs, one each for ground- based telescopes and space-based missions, and examine them using the angular spectrum Fresnel propagation module within the Physical Optics Propagation in Python (POPPY) package. We present an end-to-end (E2E) simulation of the MagAO-X instrument, an ExAO system capable of delivering 6x10 -5 visible-light raw contrast for static, noncommon path aberrations without atmosphere. We present an E2E simulation of a laser guidestar (LGS) companion spacecraft testbed demonstration, which uses a remote beacon to increase the signal available for WFS and control of the primary aperture segments of a future large space telescope, providing of order 10 factor improvement for relaxing observatory stability requirements. 2021-11-09T15:54:25Z 2021-11-09T15:54:25Z 2018-07-18 2019-10-24T15:48:38Z Article http://purl.org/eprint/type/ConferencePaper https://hdl.handle.net/1721.1/137937 Lumbres, Jennifer, Males, Jared R., Douglas, Ewan S., Close, Laird M., Cahoy, Kerri L. et al. 2018. "Modeling coronagraphic extreme wavefront control systems for high contrast imaging in ground and space telescope missions." en 10.1117/12.2313780 Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use. application/pdf SPIE SPIE |
spellingShingle | Lumbres, Jennifer Males, Jared R. Douglas, Ewan S. Close, Laird M. Cahoy, Kerri L. Carlton, Ashley K. Clark, James Doelman, David S. Feinberg, Lee D. Guyon, Olivier Knight, Justin Marlow, Weston Miller, Kelsey L. Morzinski, Katie M. Por, Emiel H. Rodack, Alexander T. Schatz, Lauren Snik, Frans Van Gorkom, Kyle Wilby, Michael J. Modeling coronagraphic extreme wavefront control systems for high contrast imaging in ground and space telescope missions |
title | Modeling coronagraphic extreme wavefront control systems for high contrast imaging in ground and space telescope missions |
title_full | Modeling coronagraphic extreme wavefront control systems for high contrast imaging in ground and space telescope missions |
title_fullStr | Modeling coronagraphic extreme wavefront control systems for high contrast imaging in ground and space telescope missions |
title_full_unstemmed | Modeling coronagraphic extreme wavefront control systems for high contrast imaging in ground and space telescope missions |
title_short | Modeling coronagraphic extreme wavefront control systems for high contrast imaging in ground and space telescope missions |
title_sort | modeling coronagraphic extreme wavefront control systems for high contrast imaging in ground and space telescope missions |
url | https://hdl.handle.net/1721.1/137937 |
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