The Magellan Telescopes: A Performance Update

The Magellan Baade and Clay telescopes regularly produce images of ~0.5" in natural seeing. We review efforts to improve collimation, active optics response, and telescope guiding and pointing to optimize the performance of the telescopes. Procedures have been developed to monitor and analyze i...

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Main Authors: Palunas, Povilas, Floyd, David, Eychaner, Glenn, Osip, David J., Schechter, Paul L.
Other Authors: Massachusetts Institute of Technology. Department of Physics
Format: Article
Language:en_US
Published: SPIE 2011
Online Access:http://hdl.handle.net/1721.1/61639
https://orcid.org/0000-0002-5665-4172
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author Palunas, Povilas
Floyd, David
Eychaner, Glenn
Osip, David J.
Schechter, Paul L.
author2 Massachusetts Institute of Technology. Department of Physics
author_facet Massachusetts Institute of Technology. Department of Physics
Palunas, Povilas
Floyd, David
Eychaner, Glenn
Osip, David J.
Schechter, Paul L.
author_sort Palunas, Povilas
collection MIT
description The Magellan Baade and Clay telescopes regularly produce images of ~0.5" in natural seeing. We review efforts to improve collimation, active optics response, and telescope guiding and pointing to optimize the performance of the telescopes. Procedures have been developed to monitor and analyze image quality delivered by the imaging science instruments. Improved models have been developed to correct for flexure of the telescope and primary mirror under gravity loading. Collimation has been improved using a "two-probe" Shack-Hartman technique to measure field aberrations. Field acquisition performance has been improved by implementing an open loop model for the primary mirror control. Telescope pointing has been improved by regular monitoring and adjustments to improve acquisition times.
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spelling mit-1721.1/616392022-09-28T15:09:08Z The Magellan Telescopes: A Performance Update Palunas, Povilas Floyd, David Eychaner, Glenn Osip, David J. Schechter, Paul L. Massachusetts Institute of Technology. Department of Physics Schechter, Paul L. Schechter, Paul L. The Magellan Baade and Clay telescopes regularly produce images of ~0.5" in natural seeing. We review efforts to improve collimation, active optics response, and telescope guiding and pointing to optimize the performance of the telescopes. Procedures have been developed to monitor and analyze image quality delivered by the imaging science instruments. Improved models have been developed to correct for flexure of the telescope and primary mirror under gravity loading. Collimation has been improved using a "two-probe" Shack-Hartman technique to measure field aberrations. Field acquisition performance has been improved by implementing an open loop model for the primary mirror control. Telescope pointing has been improved by regular monitoring and adjustments to improve acquisition times. 2011-03-09T15:42:44Z 2011-03-09T15:42:44Z 2010-07 2010-06 Article http://purl.org/eprint/type/ConferencePaper 0277-786X http://hdl.handle.net/1721.1/61639 Povilas Palunas, David Floyd, Glenn Eychaner, David J. Osip and Paul Schechter, "The Magellan Telescopes: a performance update", Proc. SPIE 7733, 77331I (2010); doi:10.1117/12.857805 © 2010 COPYRIGHT SPIE https://orcid.org/0000-0002-5665-4172 en_US http://dx.doi.org/10.1117/12.857805 Proceedings of SPIE--the International Society for Optical Engineering Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use. application/pdf SPIE SPIE
spellingShingle Palunas, Povilas
Floyd, David
Eychaner, Glenn
Osip, David J.
Schechter, Paul L.
The Magellan Telescopes: A Performance Update
title The Magellan Telescopes: A Performance Update
title_full The Magellan Telescopes: A Performance Update
title_fullStr The Magellan Telescopes: A Performance Update
title_full_unstemmed The Magellan Telescopes: A Performance Update
title_short The Magellan Telescopes: A Performance Update
title_sort magellan telescopes a performance update
url http://hdl.handle.net/1721.1/61639
https://orcid.org/0000-0002-5665-4172
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