Abstract
We introduce to astrophysical instrumentation and space optics the use of virtually imaged phased array (VIPA) to shrink échelle spectrometers and/or increase their resolution. Here, we report on both a concept of an echelle spectrometer with resolution \(R=50{,}000\) (@653nm), which fits a 6U nanosatellite platform (\({{1{\rm U}= 10\,{\rm cm} \times 10\,{\rm cm} \times 10\,{\rm cm}}}\)), and on our laboratory tests on a \(R=200{,}000\) demonstrator. The outline of our paper is as follows: Sect. 1 introduces our concept of a 6U payload comprising an échelle spectrometer based on the VIPA. We present also the science cases of monitoring young stars, and the wider science landscape amenable with larger telescopes. Section 2 gives a more detailed description of the VIPA and of its implementation in a cross-dispersed spectrometer. Section 3 shows the first results at \(R=200{,}000\) we already achieved at the Institut de Planétologie et d’Astrophysique de Grenoble (IPAG). Finally, Sect. 4 is a discussion on the remaining technical points to study.
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This research was supported by the LabEx FOCUS ANR-11-LABX-0013. The authors thank the LabEx FOCUS for its help and funding.
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This paper is based on a presentation at the International Conference on Space Optics (ICSO), October 18–21, 2016, Biarritz, France.
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Bourdarot, G., Le Coarer, E., Bonfils, X. et al. NanoVipa: a miniaturized high-resolution echelle spectrometer, for the monitoring of young stars from a 6U Cubesat. CEAS Space J 9, 411–419 (2017). https://doi.org/10.1007/s12567-017-0168-2
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DOI: https://doi.org/10.1007/s12567-017-0168-2