@inproceedings{d324775592a041feb89348d90f61c4d5,
title = "Modeling the adaptive optics systems on the Giant Magellan Telescope",
abstract = "Modeling adaptive optics (AO) systems is crucial to understanding their performance and a key aid in their design. The Giant Magellan Telescope (GMT) is planning three AO modes at first light: natural guide star AO, ground-layer AO and laser tomography AO. This paper describes how a modified version of YAO, an open-source general-purpose AO simulation tool written in Yorick, is used to simulate the GMT AO modes. The simulation tool was used to determine the piston segment error for the GMT. In addition, we present a comparison of different turbulence simulation approaches.",
keywords = "Adaptive optics, Giant magellan telescope, Simulations, Wavefront sensing",
author = "{Van Dam}, {Marcos A.} and Hinz, {Philip M.} and Codona, {Johanan L.} and Michael Hart and Aurea Garcia-Rissmann and Johns, {Matt W.} and Shectman, {Stephen A.} and Bouchez, {Antonin H.} and McLeod, {Brian A.} and Francois Rigaut",
year = "2010",
doi = "10.1117/12.856771",
language = "English",
isbn = "9780819482266",
series = "Proceedings of SPIE - The International Society for Optical Engineering",
number = "PART 1",
booktitle = "Adaptive Optics Systems II",
edition = "PART 1",
note = "Adaptive Optics Systems II ; Conference date: 27-06-2010 Through 02-07-2010",
}