Design and development of a high-speed Visible Pyramid Wavefront Sensor for the MMT AO system

被引:0
|
作者
Anugu, Narsireddy [1 ]
Durney, Olivier [1 ]
Morzinski, Katie M. [1 ]
Hinz, Phil [2 ]
Sivanandam, Suresh [3 ]
Males, Jared [1 ]
Gardner, Andrew K. [1 ]
Fellows, Chuck [4 ]
Montoya, Manny [1 ]
West, Grant [1 ]
Vaz, Amali [1 ]
Mailhot, Emily [1 ]
Carlson, Jared [1 ]
Chen, Shaojie [3 ]
Lamb, Masen [3 ]
Butko, Adam [3 ]
Downey, Elwood [1 ]
Tyler, Jacob [3 ]
Jannuzi, Buell [1 ]
机构
[1] Univ Arizona, Steward Observ, 933 N Cherry Ave, Tucson, AZ 85721 USA
[2] Univ Calif Santa Cruz, Santa Cruz 1156 High St, Santa Cruz, CA 95064 USA
[3] Univ Toronto, Dept Astron & Astrophys, 50 St George St, Toronto, ON M55 3H4, Canada
[4] Univ Arizona, Lunar & Planetary Lab, 1629 E Univ Blvd, Tucson, AZ 85721 USA
来源
ADAPTIVE OPTICS SYSTEMS VII | 2020年 / 11448卷
关键词
Adaptive optics; Adaptive secondary mirror; pyramid wavefront sensor; MMT; MAPS; ADAPTIVE OPTICS; SECONDARY;
D O I
10.1117/12.2576353
中图分类号
TM [电工技术]; TN [电子技术、通信技术];
学科分类号
0808 ; 0809 ;
摘要
MAPS, MMT Adaptive optics exoPlanet characterization System, is the upgrade of legacy 6.5m MMT adaptive optics system. It is an NSF MSIP-funded project that includes (i) refurbishing of the MMT Adaptive Secondary Mirror (ASM), (ii) new high sensitive and high spatial order visible and near-infrared pyramid wavefront sensors, and (iii) the upgrade of Arizona Infrared Imager and Echelle Spectrograph (ARIES) and MMT high Precision Imaging Polarimeter (MMTPol) science cameras. This paper will present the design and development of the visible pyramid wavefront sensor. This system consists of an acquisition camera, a fast-steering tip-tilt modulation mirror, a double pyramid, a pupil imaging triplet lens, and a low noise and high-speed frame rate based CCID75 camera. We will report on hardware and software and present the laboratory characterization results of the individual subsystems, and outline the on-sky commissioning plan.
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页数:16
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