Paper
15 July 2010 The first VisAO-fed integral field spectrograph: VisAO IFS
Author Affiliations +
Abstract
We present the optomechanical design of the Magellan VisAO Integral Field Spectrograph (VisAO IFS), designed to take advantage of Magellan's AO system and its 85.1cm concave ellipsoidal Adaptive Secondary Mirror (ASM). With 585 actuators and an equal number of actively-controlled modes, this revolutionary second generation ASM will be the first to achieve moderate Strehl ratios into the visible wavelength regime. We have designed the VisAO IFS to be coupled to either Magellan's LDSS-3 spectrograph or to the planned facility M2FS fiber spectrograph and to optimize VisAO science. Designed for narrow field-of-view, high spatial resolution science, this lenslet-coupled fiberfed IFS will offer exciting opportunities for scientific advancement in a variety of fields, including protoplanetary disk morphology and chemistry, resolution and spectral classification of tight astrometric binaries, seasonal changes in the upper atmosphere of Titan, and a better understanding of the black hole M-sigma relation.
© (2010) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Katherine B Follette, Laird M. Close, Derek Kopon, Jared R. Males, Victor Gasho, Kevin M. Brutlag, and Alan Uomoto "The first VisAO-fed integral field spectrograph: VisAO IFS", Proc. SPIE 7735, Ground-based and Airborne Instrumentation for Astronomy III, 77351P (15 July 2010); https://doi.org/10.1117/12.857516
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Cited by 2 scholarly publications.
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KEYWORDS
Iterated function systems

Spectrographs

Adaptive optics

Stars

Spectral resolution

Spatial resolution

Atmospheric modeling

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