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NFIRAOS: TMT facility adaptive optics with conventional DMs.

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Title: NFIRAOS: TMT facility adaptive optics with conventional DMs.
Author: Hickson, Paul
Issue Date: 2005
Publicly Available in cIRcle 2011-09-20
Publisher Society of Photo-Optical Instrumentation Engineers
Citation: Herriot, Glen; Hickson, Paul; Ellerbroek, Brent L.; Andersen, David A.; Davidge, Timothy; Erickson, David A.; Powell, Ian P.; Clare, Richard M.; Smith, Malcolm; Saddlemyer, Leslie: and J.-P. Veran, NFIRAOS: TMT facility adaptive optics with conventional DMs. Astronomical Adaptive Optics Systems and Applications II, edited by Robert K. Tyson, Michael Lloyd-Hart. Proceedings of SPIE Volume 5903, 590302, 2005. http://dx.doi.org/10.1117/12.617849
Abstract: Although many of the instruments planned for the TMT (Thirty Meter Telescope) have their own closely-coupled adaptive optics systems, TMT will also have a facility Adaptive Optics (AO) system feeding three instruments on the Nasmyth platform. For this Narrow-Field Infrared Adaptive Optics System, NFIRAOS (pronounced nefarious), the TMT project considered two architectures. One, described in this paper, employs conventional deformable mirrors with large diameters of about 300 mm and this is the reference design adopted by the TMT project. An alternative design based on MEMS was also studied, and is being presented separately in this conference. The requirements for NFIRAOS include 0.8-5 microns wavelength range, 30 arcsecond diameter output field of view (FOV), excellent sky coverage, and diffraction-limited atmospheric turbulence compensation (specified at 133 nm RMS including residual telescope and science instrument errors.) The reference design for NFIRAOS includes multiple sodium laser guide stars over a 70 arcsecond FOV, and an infrared tip/tilt/focus/astigmatism natural guide star sensor within instruments. Larger telescopes require greater deformable mirror (DM) stroke. Although initially NFIRAOS will correct a 10 arcsecond science field, it uses two deformable mirrors in series, partly to provide sufficient stroke for atmospheric correction over the 30 m telescope aperture, but mainly to partially correct a 2 arcminute diameter "technical" field to sharpen near-IR natural guide stars and improve sky coverage. The planned upgrade to full performance includes replacing the ground conjugated DM with a higher actuator density, and using a deformable telescope secondary mirror as a "woofer." NFIRAOS incorporates an instrument rotator and selection of three live instruments: a near-Infrared integral field Imaging spectrograph, a near-infrared echelle spectrograph, and after upgrading NFIRAOS to full multi-conjugation, a wide field (30 arcsecond) infrared camera. Copyright 2005 Society of Photo-Optical Instrumentation Engineers. One print or electronic copy may be made for personal use only. Systematic reproduction and distribution, duplication of any material in this paper for a fee or for commercial purposes, or modification of the content of the paper are prohibited.
Affiliation: Science, Faculty ofPhysics and Astronomy, Department of
URI: http://hdl.handle.net/2429/37485
Peer Review Status: Reviewed
Scholarly Level: Faculty

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