GSMT Program Office
Working Towards a Giant Segmented Mirror Telescope
As of May, 2009, these pages are no longer being actively
maintained. For up-to-date information, please see the NOAO System Page at: http://ast.noao.edu/system/.
SPIE Conference
Waikoloa, Hawaii
August 22 - 28, 2002
SPIE Papers Submitted
- J. Najita and S. E. Strom, National Optical Astronomy Observatory, Science enabled by a 30-m telescope
- Stephen E. Strom, Larry Stepp, Brooke Gregory, AURA New Initiatives Office, Giant Segmented Mirror Telescope: a point design based on science drivers
- Stephen E. Strom, Larry Stepp, Brooke Gregory, AURA New Initiatives Office, A Science-Driven GSMT Point Design - presentation
- Larry Stepp, Larry Daggert, and Paul Gillett, AURA New Initiatives Office and National Optical Astronomy Observatory, Estimating the Costs of Extremely Large Telescopes
- Larry Stepp, Larry Daggert, and Paul Gillett, AURA New Initiatives Office and National Optical Astronomy Observatory, Estimating the Costs of Extremely Large Telescopes - presentation
- M. Whorton, G. Angeli, NASA Marshall Space Flight Center/Tennessee State University and AURA New Initiatives Office, Modern Control for the Secondary Mirror of a Giant Segmented Mirror Telescope
- M. Whorton, G. Angeli, NASA Marshall Space Flight Center/Tennessee State University and AURA New Initiatives Office, Modern Control for the Secondary Mirror of a Giant Segmented Mirror Telescope- charts
- George Z. Angeli, Myung K. Cho, Mark S. Whorton, AURA New Initiatives Office and NASA Marshall Space Flight Center, Active Optics and Control Architecture for a Giant Segmented Mirror Telescope
- George Z. Angeli, Myung K. Cho, Mark S. Whorton, AURA New Initiatives Office and NASA Marshall Space Flight Center,Active Optics and Control Architecture for a Giant Segmented Mirror Telescope - presentation
- Guanpeng Xu, Mark Whorton, Yong X.Tao, Myung Cho, Tennessee State University, NASA, Florida International University, AURA New Initiatives Office, Dynamic Modeling of Turbulent Shedding Effect on the 30-meter Primary Mirror of GSMT
- Guanpeng Xu, Mark Whorton, Yong X.Tao, Myung Cho, Tennessee State University, NASA, Florida International University, AURA New Initiatives Office, Dynamic Modeling of Turbulent Shedding Effect on the 30-meter Primary Mirror of GSMT - poster
- Myung Cho, Larry Stepp, George Angeli, David Smith, AURA New Initiatives Office and MERLAB, Wind Loading of Large Telescopes - presentation
- Myung Cho, Larry Stepp, George Angeli, David Smith, AURA New Initiatives Office and MERLAB, Wind Loading of Large Telescopes
- Brent L. Ellerbroek, L. Gilles, and C. R. Vogel, Gemini Observatory, Michigan Technical University, and Montana State University, A Computationally Efficient Wavefront Reconstructor for Simulations of Multi-Conjugate Adaptive Optics on Giant Telescopes
- Brent Ellerbroek and Richard Buchroeder, Gemini Observatory and Optical Design Service, Near-Infrared AO Coronagraph Design for Giant Telescopes
- L. Gilles, B.L.Ellerbroek, and C.R. Vogel, Michigan Technological University, Gemini Observatory, and Montana State University, Layer-Oriented multigrid Wavefront Reconstruction Algorithms for Multi-Conjugate Adaptive Optics
- Alistair R. Walker, Robert E. Blum, Maxime Boccas, Edison Bustos, Hugo E. Schwarz, Nicholas B. Suntzeff, and Andrei Tokovinin, Site Survey for the Giant Segmented Mirror Telescope