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Proceedings Article

Science instrument development for the Giant Magellan Telescope

[+] Author Affiliations
D. T. Jaffe

The Univ. of Texas at Austin (USA)

D. L. DePoy

Texas A&M Univ. (USA)

D. G. Fabricant, A. Szentgyorgyi

Harvard-Smithsonian Ctr. for Astrophysics (USA)

P. M. Hinz

The Univ. of Arizona (USA)

G. Jacoby, M. Johns, P. McCarthy

GMTO Corp. (USA)

P. J. McGregor

The Australian National Univ. (Australia)

S. Shectman

Carnegie Institution for Science (USA)

Proc. SPIE 7735, Ground-based and Airborne Instrumentation for Astronomy III, 773525 (July 15, 2010); doi:10.1117/12.856619
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From Conference Volume 7735

  • Ground-based and Airborne Instrumentation for Astronomy III
  • Ian S. McLean; Suzanne K. Ramsay; Hideki Takami
  • San Diego, California, USA | June 27, 2010

abstract

The Giant Magellan Telescope (GMT) is a 24.5m diameter optical/infrared telescope. Its seven 8.4m primary mirrors give it a collecting area equivalent to a 21.4m filled aperture. The ten GMT partners are constructing the telescope at the Las Campanas Observatory in Chile with first light planned for the end of 2018. In this paper, we describe the plans for the first-generation focal plane instrumentation for the telescope. The GMTO Corporation has solicited studies for instruments capable of carrying out the broad range of objectives outlined in the GMT Science Case. Six instruments have been selected for 14 month long conceptual design studies. We briefly describe the features of these instruments and give examples of the major science questions that they can address.

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

D. T. Jaffe ; D. L. DePoy ; D. G. Fabricant ; P. M. Hinz ; G. Jacoby, et al.
"Science instrument development for the Giant Magellan Telescope", Proc. SPIE 7735, Ground-based and Airborne Instrumentation for Astronomy III, 773525 (July 15, 2010); doi:10.1117/12.856619; http://dx.doi.org/10.1117/12.856619


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