High contrast imaging with the Magellan VisAO camera

Jared R. Males; Laird M. Close; Katie M. Morzinski; Derek Kopon; Katherine B. Follette; Philip M. Hinz; Timothy J. Rodigas; Alfio Puglisi; Simone Esposito; Armando Riccardi; Enrico Pinna; Marco Xompero; Runa Briguglio; Ya Lin Wu; Alan Uomoto; Tyson Hare

doi:10.12839/AO4ELT3.13286

High contrast imaging with the Magellan VisAO camera

Jared R. Males, Laird M. Close, Katie M. Morzinski, Derek Kopon, Katherine B. Follette, Philip M. Hinz, Timothy J. Rodigas, Alfio Puglisi, Simone Esposito, Armando Riccardi, Enrico Pinna, Marco Xompero, Runa Briguglio, Ya Lin Wu, Alan Uomoto, Tyson Hare

研究成果: 書貢獻/報告類型 › 會議論文篇章

2 引文斯高帕斯（Scopus）

摘要

The Magellan Adaptive Optics system (MagAO) saw first light in November 2012 at Las Campanas Observatory on the 6.5m Clay telescope. Here we present an introduction to MagAO's visible wavelength diffraction limited imager, VisAO. VisAO delivers Strehl ratios greater than 30% from 0.62 microns (r') through 1 micron, where Strehl is even higher, and achieved resolutions as small as 20 milli-arcseconds. There are several design considerations which allow VisAO to achieve such good performance on a large telescope, and these will have important implications for ELT AO systems. We took advantage of the excellent performance of MagAO/VisAO to conduct high contrast observations of an exoplanet in the optical.

原文	英語
主出版物標題	3rd AO4ELT Conference - Adaptive Optics for Extremely Large Telescopes
發行者	INAF - Osservatorio Astrofisico di Arcetri Largo Enrico Fermi
ISBN（列印）	9788890887604
DOIs	https://doi.org/10.12839/AO4ELT3.13286
出版狀態	已發佈 - 2013
對外發佈	是
事件	3rd Conference on Adaptive Optics for Extremely Large Telescopes, AO4ELT 2013 - Florence, 意大利持續時間: 2013 5月 26 → 2013 5月 31

出版系列

名字	3rd AO4ELT Conference - Adaptive Optics for Extremely Large Telescopes

會議

會議	3rd Conference on Adaptive Optics for Extremely Large Telescopes, AO4ELT 2013
國家/地區	意大利
城市	Florence
期間	2013/05/26 → 2013/05/31

ASJC Scopus subject areas

原子與分子物理與光學
電子、光磁材料

存取文件

10.12839/AO4ELT3.13286

其它文件與鏈接

引用此

Males, J. R., Close, L. M., Morzinski, K. M., Kopon, D., Follette, K. B., Hinz, P. M., Rodigas, T. J., Puglisi, A., Esposito, S., Riccardi, A., Pinna, E., Xompero, M., Briguglio, R., Wu, Y. L., Uomoto, A., & Hare, T. (2013). High contrast imaging with the Magellan VisAO camera. 於 3rd AO4ELT Conference - Adaptive Optics for Extremely Large Telescopes (3rd AO4ELT Conference - Adaptive Optics for Extremely Large Telescopes). INAF - Osservatorio Astrofisico di Arcetri Largo Enrico Fermi. https://doi.org/10.12839/AO4ELT3.13286

High contrast imaging with the Magellan VisAO camera. / Males, Jared R.; Close, Laird M.; Morzinski, Katie M. 等.
3rd AO4ELT Conference - Adaptive Optics for Extremely Large Telescopes. INAF - Osservatorio Astrofisico di Arcetri Largo Enrico Fermi, 2013. (3rd AO4ELT Conference - Adaptive Optics for Extremely Large Telescopes).

研究成果: 書貢獻/報告類型 › 會議論文篇章

Males, JR, Close, LM, Morzinski, KM, Kopon, D, Follette, KB, Hinz, PM, Rodigas, TJ, Puglisi, A, Esposito, S, Riccardi, A, Pinna, E, Xompero, M, Briguglio, R, Wu, YL, Uomoto, A & Hare, T 2013, High contrast imaging with the Magellan VisAO camera. 於 3rd AO4ELT Conference - Adaptive Optics for Extremely Large Telescopes. 3rd AO4ELT Conference - Adaptive Optics for Extremely Large Telescopes, INAF - Osservatorio Astrofisico di Arcetri Largo Enrico Fermi, 3rd Conference on Adaptive Optics for Extremely Large Telescopes, AO4ELT 2013, Florence, 意大利, 2013/05/26. https://doi.org/10.12839/AO4ELT3.13286

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title = "High contrast imaging with the Magellan VisAO camera",

abstract = "The Magellan Adaptive Optics system (MagAO) saw first light in November 2012 at Las Campanas Observatory on the 6.5m Clay telescope. Here we present an introduction to MagAO's visible wavelength diffraction limited imager, VisAO. VisAO delivers Strehl ratios greater than 30% from 0.62 microns (r') through 1 micron, where Strehl is even higher, and achieved resolutions as small as 20 milli-arcseconds. There are several design considerations which allow VisAO to achieve such good performance on a large telescope, and these will have important implications for ELT AO systems. We took advantage of the excellent performance of MagAO/VisAO to conduct high contrast observations of an exoplanet in the optical.",

author = "Males, {Jared R.} and Close, {Laird M.} and Morzinski, {Katie M.} and Derek Kopon and Follette, {Katherine B.} and Hinz, {Philip M.} and Rodigas, {Timothy J.} and Alfio Puglisi and Simone Esposito and Armando Riccardi and Enrico Pinna and Marco Xompero and Runa Briguglio and Wu, {Ya Lin} and Alan Uomoto and Tyson Hare",

year = "2013",

doi = "10.12839/AO4ELT3.13286",

language = "English",

isbn = "9788890887604",

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T1 - High contrast imaging with the Magellan VisAO camera

AU - Males, Jared R.

AU - Close, Laird M.

AU - Morzinski, Katie M.

AU - Kopon, Derek

AU - Follette, Katherine B.

AU - Hinz, Philip M.

AU - Rodigas, Timothy J.

AU - Puglisi, Alfio

AU - Esposito, Simone

AU - Riccardi, Armando

AU - Pinna, Enrico

AU - Xompero, Marco

AU - Briguglio, Runa

AU - Wu, Ya Lin

AU - Uomoto, Alan

AU - Hare, Tyson

PY - 2013

Y1 - 2013

N2 - The Magellan Adaptive Optics system (MagAO) saw first light in November 2012 at Las Campanas Observatory on the 6.5m Clay telescope. Here we present an introduction to MagAO's visible wavelength diffraction limited imager, VisAO. VisAO delivers Strehl ratios greater than 30% from 0.62 microns (r') through 1 micron, where Strehl is even higher, and achieved resolutions as small as 20 milli-arcseconds. There are several design considerations which allow VisAO to achieve such good performance on a large telescope, and these will have important implications for ELT AO systems. We took advantage of the excellent performance of MagAO/VisAO to conduct high contrast observations of an exoplanet in the optical.

AB - The Magellan Adaptive Optics system (MagAO) saw first light in November 2012 at Las Campanas Observatory on the 6.5m Clay telescope. Here we present an introduction to MagAO's visible wavelength diffraction limited imager, VisAO. VisAO delivers Strehl ratios greater than 30% from 0.62 microns (r') through 1 micron, where Strehl is even higher, and achieved resolutions as small as 20 milli-arcseconds. There are several design considerations which allow VisAO to achieve such good performance on a large telescope, and these will have important implications for ELT AO systems. We took advantage of the excellent performance of MagAO/VisAO to conduct high contrast observations of an exoplanet in the optical.

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DO - 10.12839/AO4ELT3.13286

M3 - Conference contribution

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SN - 9788890887604

T3 - 3rd AO4ELT Conference - Adaptive Optics for Extremely Large Telescopes

BT - 3rd AO4ELT Conference - Adaptive Optics for Extremely Large Telescopes

PB - INAF - Osservatorio Astrofisico di Arcetri Largo Enrico Fermi

T2 - 3rd Conference on Adaptive Optics for Extremely Large Telescopes, AO4ELT 2013

Y2 - 26 May 2013 through 31 May 2013

ER -

High contrast imaging with the Magellan VisAO camera

摘要

出版系列

會議

ASJC Scopus subject areas

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其它文件與鏈接

指紋

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