Enabling high resolution visible AO at the W.M. Keck Observatory Article Swipe
Eduardo Marín
,
Peter Wizinowich
,
Maxwell A. Millar‐Blanchaer
,
Eliad Peretz
,
Sam Ragland
,
Marc-André Boucher
,
Jason Chin
,
Guillaume Filon
,
J. Fowler
,
Luke Gers
,
Jack J. Grossman
,
Shui Kwok
,
Jean Thomas Landry
,
Scott Lilley
,
Bert A. Pasquale
,
Ed Wetherell
,
Rebecca Jensen-Clem
,
Imke de Parker
,
Etienne Gauvin
,
Kevin Hall
,
Peter Kurczynski
,
John Mather
,
E. Nielsen
,
Lucas Parbacius
,
Peter Plavchan
,
Steph Sallum
,
Shobita Satyapal
·
YOU?
·
· 2023
· Open Access
·
· DOI: https://doi.org/10.13009/ao4elt7-2023-031
YOU?
·
· 2023
· Open Access
·
· DOI: https://doi.org/10.13009/ao4elt7-2023-031
The W. M. Keck Observatory has generated an observatory wide strategic plan for 2035. This plan has identified visible Adaptive Optics (AO) as an attractive science path for the observatory. Given the 10-meter aperture of the Keck telescopes, a visible AO system can achieve extremely high spatial resolutions. These high resolutions will be comparable to that of Extremely Large Telescopes (ELTs) in the infrared, which can lead to synergistic observations between the observatories. To demonstrate the feasibility of visible AO we have recently installed a visible camera (ORKID) that works behind AO as part of the ORbiting Configurable Artificial Stars (ORCAS) mission. ORCAS is a first-of-its-kind hybrid space and ground observatory, using a satellite-based laser as the AO beacon for wavefront sensing. As a risk reduction for ORCAS we have demonstrated the opportunistic use of a passing asteroid (known as an appulse) as a source for AO wavefront sensing on UGC 4729, an object where there is no viable nature guide star for AO observations. To demonstrate the angular resolution of the Keck telescopes at visible wavelengths we have used the ORKID camera to image a number of targets including the close binary Theta Orionis C. The binary is detected at a separation of 44.4 mas, with a FWHM of 15.1 mas at 650nm. This is the sharpest point spread function (PSF) ever measured at Keck demonstrating the potential offered by visible AO. These two demonstrations show the potential for high resolution visible AO science. We present the rational for pushing to the visible, results from ORKID, results of our appulse demonstration, and our AO development plans that will enable high resolution visible AO at the W.M. Keck Observatory.
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- Type
- article
- Language
- en
- Landing Page
- https://hal.science/hal-04402847
- OA Status
- green
- Related Works
- 10
- OpenAlex ID
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Raw OpenAlex JSON
- OpenAlex ID
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- DOI
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https://doi.org/10.13009/ao4elt7-2023-031Digital Object Identifier
- Title
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Enabling high resolution visible AO at the W.M. Keck ObservatoryWork title
- Type
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articleOpenAlex work type
- Language
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enPrimary language
- Publication year
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2023Year of publication
- Publication date
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2023-01-01Full publication date if available
- Authors
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Eduardo Marín, Peter Wizinowich, Maxwell A. Millar‐Blanchaer, Eliad Peretz, Sam Ragland, Marc-André Boucher, Jason Chin, Guillaume Filon, J. Fowler, Luke Gers, Jack J. Grossman, Shui Kwok, Jean Thomas Landry, Scott Lilley, Bert A. Pasquale, Ed Wetherell, Rebecca Jensen-Clem, Imke de Parker, Etienne Gauvin, Kevin Hall, Peter Kurczynski, John Mather, E. Nielsen, Lucas Parbacius, Peter Plavchan, Steph Sallum, Shobita SatyapalList of authors in order
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https://hal.science/hal-04402847Publisher landing page
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YesWhether a free full text is available
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greenOpen access status per OpenAlex
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https://hal.science/hal-04402847Direct OA link when available
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Observatory, Physics, Remote sensing, Optics, Astronomy, GeologyTop concepts (fields/topics) attached by OpenAlex
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0Total citation count in OpenAlex
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10Other works algorithmically related by OpenAlex
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