Presentation + Paper
21 August 2020 New spectro-imager designs for MOEMS-based instruments in Earth and Universe observation
Author Affiliations +
Abstract
MOEMS-based instruments could be the next stepping stone for ground-based and space telescopes, allowing for multi-object spectroscopy in a 2D field of view. These programmable slit masks will optimize the SNR and generate compact and efficient spectro-imagers for Universe and Earth observation. BATMAN, a MOEMS-based spectro-imager for Universe observation to be installed at the TNG at the Canaria Islands, uses a Digital-Micromirror-Device to split the light between its imaging and spectrograph arms. ROBIN, the BATMAN demonstrator, confirmed its feasibility and image quality over the FOV. A new design for a DMD-based high-resolution spectro-imager for Universe observation is presented: a solution using only one detector for all the wavelength range is obtained. We are dividing the 370 – 950 nm wavelength range into four channels and a spectral resolution of 15 000 is achieved for every one of them, all within an image quality below two detector pixels. Moreover, the 3-mirror design of the instrument implies a high throughput in comparison to catadioptric systems which are more commonly used for this science case. A new MOEMS-based spectro-imager for Earth observation has been designed, with constraints of wide 2D field of view (3°×1°), image quality (< 2 pixels = 11 μm) and compacity. The instrument is panchromatic with a medium spectral resolution between 1000 and 2000, fitting in a 40 cm × 50 cm × 90 cm box. A 3-mirror solution for both imaging and spectrograph arms has been designed, using only aspheric surfaces thus allowing for easier alignment and tolerancing.
Conference Presentation
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Mathieu Vachey, Frédéric Zamkotsian, Vincent Costes, Hervé Benard, Arnaud Liotard, and Nicolas Tetaz "New spectro-imager designs for MOEMS-based instruments in Earth and Universe observation", Proc. SPIE 11483, Novel Optical Systems, Methods, and Applications XXIII, 1148308 (21 August 2020); https://doi.org/10.1117/12.2569670
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KEYWORDS
Spectrographs

Spectral resolution

Imaging systems

Telescopes

Image quality

Digital micromirror devices

Micromirrors

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