Paper
7 March 2003 Visible Imaging Fourier Transform Spectrometer: Design and Calibration
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Abstract
We present details of the design, operation and calibration of an astronomical visible-band imaging Fourier transform spectrometer (IFTS). This type of instrument produces a spectrum for every pixel in the field of view where the spectral resolution is flexible. The instrument is a dual-input/dual-output Michelson interferometer coupled to the 3.5 meter telescope at the Apache Point Observatory. Imaging performance, and interferograms and spectra from calibration sources and standard stars are discussed.
© (2003) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Edward H. Wishnow, Ronald E. Wurtz, Sebastien Blais-Ouellette, Kem Holland Cook, Dennis J. Carr, Isabella T. Lewis, Frederic Grandmont, and Christopher W. Stubbs "Visible Imaging Fourier Transform Spectrometer: Design and Calibration", Proc. SPIE 4841, Instrument Design and Performance for Optical/Infrared Ground-based Telescopes, (7 March 2003); https://doi.org/10.1117/12.461512
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Cited by 5 scholarly publications.
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KEYWORDS
Interferometers

Cameras

Mirrors

Telescopes

Spectroscopy

Stars

Visibility

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