GMT overview

The 25-meter Giant Magellan Telescope (GMT) is one of the next generation of extremely large ground-based optical/infrared telescopes. GMT is currently under development by a consortium of major US and international university and research institutions. The telescope will be located at the Las Campanas Observatory in Chile. The GMT Project is mid-way through its Design Development Phase. This paper summarizes the organizational structure and status of the GMT Project and recent progress in the technical development of the various GMT subsystems.

[1]  Matt Johns,et al.  Giant Magellan Telescope site testing: summary , 2010, Astronomical Telescopes + Instrumentation.

[2]  Roberto Biasi,et al.  GMT adaptive secondary design , 2010, Astronomical Telescopes + Instrumentation.

[3]  Tom L. Zobrist,et al.  Accuracy of laser tracker measurements of the GMT 8.4 m off-axis mirror segments , 2010, Astronomical Telescopes + Instrumentation.

[4]  Catherine Mayumi Ohara,et al.  Phasing the primary mirror segments of the Keck telescopes: a comparison of different techniques , 2000, Astronomical Telescopes and Instrumentation.

[5]  Patrick McCarthy,et al.  Giant Magellan Telescope site testing: PWV statistics and calibration , 2010, Astronomical Telescopes + Instrumentation.

[6]  Philip M. Hinz,et al.  Modeling adaptive optics for the segmented aperture of the GMT , 2010, Astronomical Telescopes + Instrumentation.

[7]  Stephen A. Shectman,et al.  Modeling the adaptive optics systems on the Giant Magellan Telescope , 2010, Astronomical Telescopes + Instrumentation.

[8]  James H. Burge,et al.  Scanning pentaprism test for the GMT 8.4-m off-axis segments , 2010, Astronomical Telescopes + Instrumentation.

[9]  In-Soo Yuk,et al.  GMTNIRS (Giant Magellan Telescope near-infrared spectrograph): design concept , 2010, Astronomical Telescopes + Instrumentation.

[10]  Tom L. Zobrist,et al.  Fabrication and testing of the first 8.4-m off-axis segment for the Giant Magellan Telescope , 2010, Astronomical Telescopes + Instrumentation.

[11]  Matt Johns Progress on the GMT , 2008, Astronomical Telescopes + Instrumentation.

[12]  Matt Johns,et al.  Giant Magellan Telescope primary mirror cells , 2010, Astronomical Telescopes + Instrumentation.

[13]  Tom L. Zobrist,et al.  Alignment and use of the optical test for the 8.4-m off-axis primary mirrors of the Giant Magellan Telescope , 2010, Astronomical Telescopes + Instrumentation.

[14]  Matthew Colless,et al.  MANIFEST: a many-instrument fiber-positioning system for GMT , 2010, Astronomical Telescopes + Instrumentation.

[15]  Michael Hart,et al.  The GMT adaptive optics system , 2010, Astronomical Telescopes + Instrumentation.

[16]  Matt Johns,et al.  Giant Magellan Telescope site testing seeing and turbulence statistics , 2010, Astronomical Telescopes + Instrumentation.

[17]  D. L. DePoy,et al.  Science instrument development for the Giant Magellan Telescope , 2010, Astronomical Telescopes + Instrumentation.

[18]  Steve Gunnels The Giant Magellan Telescope (GMT): hydrostatic constraints , 2010, Astronomical Telescopes + Instrumentation.