ORCAS Keck instrument demonstrator

The Orbiting Configurable Artificial Star (ORCAS) mission in collaboration with the W. M. Keck Observatory has designed, assembled, built, and delivered, within 180 days, ORCAS Keck Instrument Demonstrator (ORKID) (ORCAS Keck Instrument Demonstrator), an early visible-wavelength performance demonstration with the Keck II Adaptive Optics (AO) system. The optical performance of ORKID meets the technical requirements derived from the scientific goals of having a Nyquist-sampled point spread function at 650 nm. This is achieved by diffraction-limited as-built performance with a root mean square internal wavefront error below 50 nm, which is key for the advancement of the ORCAS mission. ORKID has acquired, with a closed AO loop, no frame selection, while shifting and adding, the sharpest-ever on-sky image captured at Keck II. With a full width at half maximum of ∼15 mas, this is the equivalent of a 9-m diffraction-limited telescope. By doing so, the immense potential and viability of the proposed Hybrid Observatory ORCAS mission are demonstrated.

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Publication Details

Journal
Journal of Astronomical Telescopes Instruments and Systems
Published
2025-03-28
DOI
https://doi.org/10.1117/1.jatis.11.1.014004
Primary Topic
Particle Accelerators and Free-Electron Lasers
Type
article
Field-Weighted Citation Impact
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article

ORCAS Keck instrument demonstrator

Peter Kurczynski, Maxwell A. Millar‐Blanchaer, J. Fowler, Eliad Peretz et al.
Journal of Astronomical Telescopes Instruments and Systems
Particle Accelerators and Free-Electron Lasers
article

ORCAS Keck instrument demonstrator

Peter Kurczynski, Maxwell A. Millar‐Blanchaer, J. Fowler, Eliad Peretz, Guillaume Filion, Peter Plavchan, E. Nielsen, Jason Chin, Rebecca Jensen-Clem, Marc Kassis, Scott Lilley, Ed Wetherell, Vivian Palmer, Luke Gers, Kevin Hall, Sam Ragland, Steph Sallum, John M. O’Meara, Peter Wizinowich, Étienne Gauvin, Andrew Lewis, Imke de Pater, Eduardo Marín, Shobita Satyapal, Shui Kwok, Kayla Carmical, Maya Wertheim, Jack J. Grossman, Jean Thomas Landry, John Mather, Brett Smith, Bert A. Pasquale
article en

Abstract

The Orbiting Configurable Artificial Star (ORCAS) mission in collaboration with the W. M. Keck Observatory has designed, assembled, built, and delivered, within 180 days, ORCAS Keck Instrument Demonstrator (ORKID) (ORCAS Keck Instrument Demonstrator), an early visible-wavelength performance demonstration with the Keck II Adaptive Optics (AO) system. The optical performance of ORKID meets the technical requirements derived from the scientific goals of having a Nyquist-sampled point spread function at 650 nm. This is achieved by diffraction-limited as-built performance with a root mean square internal wavefront error below 50 nm, which is key for the advancement of the ORCAS mission. ORKID has acquired, with a closed AO loop, no frame selection, while shifting and adding, the sharpest-ever on-sky image captured at Keck II. With a full width at half maximum of ∼15 mas, this is the equivalent of a 9-m diffraction-limited telescope. By doing so, the immense potential and viability of the proposed Hybrid Observatory ORCAS mission are demonstrated.

Journal of Astronomical Telescopes Instruments and SystemsVol. 11(01)
New Mexico State University (US), Goddard Space Flight Center (US), University of California, Santa Barbara (US), George Mason University (US), University of California, Santa Cruz (US), University of California, Irvine (US), W.M. Keck Observatory (US), University of California, Berkeley (US)
Openalex Percentile: Top 95%
Particle Accelerators and Free-Electron Lasers
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