Science instrument development for the Giant Magellan Telescope

D. T. Jaffe, D. L. DePoy, D. G. Fabricant, P. M. Hinz, G. Jacoby, M. Johns, P. McCarthy, P. J. McGregor, S. Shectman, A. Szentgyorgyi

    Research output: Chapter in Book/Report/Conference proceedingConference contributionpeer-review

    5 Citations (Scopus)

    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.

    Original languageEnglish
    Title of host publicationGround-Based and Airborne Instrumentation for Astronomy III
    EditionPART 1
    DOIs
    Publication statusPublished - 2010
    EventGround-Based and Airborne Instrumentation for Astronomy III - San Diego, CA, United States
    Duration: 27 Jun 20102 Jul 2010

    Publication series

    NameProceedings of SPIE - The International Society for Optical Engineering
    NumberPART 1
    Volume7735
    ISSN (Print)0277-786X

    Conference

    ConferenceGround-Based and Airborne Instrumentation for Astronomy III
    Country/TerritoryUnited States
    CitySan Diego, CA
    Period27/06/102/07/10

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