Full Content is available to subscribers

Subscribe/Learn More  >
Proceedings Article

The Magellan Telescope Adaptive Secondary AO System: a visible and mid-IR AO facility

[+] Author Affiliations
Laird M. Close, Victor Gasho, Derek Kopon, Jared Males, Katherine B. Follette, Kevin Brutlag

Steward Observatory, The Univ. of Arizona (USA)

Alan Uomoto, Tyson Hare

Carnegie Observatories (USA)

Proc. SPIE 7736, Adaptive Optics Systems II, 773605 (July 14, 2010); doi:10.1117/12.857924
Text Size: A A A
From Conference Volume 7736

  • Adaptive Optics Systems II
  • Brent L. Ellerbroek; Michael Hart; Norbert Hubin; Peter L. Wizinowich
  • San Diego, California, USA | June 27, 2010

abstract

The Magellan Clay telescope is a 6.5m Gregorian telescope located in Chile at Las Campanas Observatory. The Gregorian design allows for an adaptive secondary mirror that can be tested off-sky in a straightforward manner. We have fabricated a 85 cm diameter aspheric adaptive secondary with our subcontractors and partners, the ASM passed acceptance tests in July 2010. This secondary has 585 actuators with <1 msec response times (0.7 ms typically). This adaptive secondary will allow low emissivity AO science. We will achieve very high Strehls (~98%) in the Mid-IR (3-26 microns) with the BLINC/MIRAC4 Mid-IR science camera. This will allow the first "super-resolution" and nulling Mid-IR studies of dusty southern objects. We will employ a high order (585 mode) pyramid wavefront sensor similar to that now successfully used at the Large Binocular Telescope. The relatively high actuator count will allow modest Strehls to be obtained in the visible (0.63-1.05 μm). Moderate (~20%) Strehls have already been obtained at 0.8 μm at the LBT with the same powerful combination of a next generation ASM and Pyramid WFS as we are providing for Magellan. Our visible light AO (VisAO) science camera is fed by an advanced triplet ADC and is piggy-backed on the WFS optical board. We have designed an additional "clean-up" very fast (2 kHz) tilt stabilization system for VisAO. Also a high-speed shutter will be used to block periods of poor correction. The VisAO facility can be reconfigured to feed an optical IFU spectrograph with 20 mas spaxels. The entire system passed CDR in June 2009, and is now finished the fabrication phase and is entering the integration phase. The system science and performance requirements, and an overview the design, interface and schedule for the Magellan AO system are presented here.

© (2010) COPYRIGHT SPIE--The International Society for Optical Engineering. Downloading of the abstract is permitted for personal use only.
Citation

Laird M. Close ; Victor Gasho ; Derek Kopon ; Jared Males ; Katherine B. Follette, et al.
"The Magellan Telescope Adaptive Secondary AO System: a visible and mid-IR AO facility", Proc. SPIE 7736, Adaptive Optics Systems II, 773605 (July 14, 2010); doi:10.1117/12.857924; http://dx.doi.org/10.1117/12.857924


Access This Proceeding
Sign in or Create a personal account to Buy this proceeding ($15 for members, $18 for non-members).

Figures

Tables

NOTE:
Citing articles are presented as examples only. In non-demo SCM6 implementation, integration with CrossRef’s "Cited By" API will populate this tab (http://www.crossref.org/citedby.html).

Some tools below are only available to our subscribers or users with an online account.

Related Content

Customize your page view by dragging & repositioning the boxes below.

Related Book Chapters

Topic Collections

Advertisement


  • Don't have an account?
  • Subscribe to the SPIE Digital Library
  • Create a FREE account to sign up for Digital Library content alerts and gain access to institutional subscriptions remotely.
Access This Proceeding
Sign in or Create a personal account to Buy this proceeding ($15 for members, $18 for non-members).
Access This Proceeding
Sign in or Create a personal account to Buy this article ($15 for members, $18 for non-members).
Access This Chapter

Access to SPIE eBooks is limited to subscribing institutions and is not available as part of a personal subscription. Print or electronic versions of individual SPIE books may be purchased via SPIE.org.