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Simulating the Retrieval of Astronomical Spectra from the SPICA SAFARI Post Dispersed Fourier Transform Spectrometer

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Abstract

The SPICA mission will employ ultra-sensitive superconducting detectors. In this case the multiplex disadvantage of Fourier transform spectroscopy dictates the use of a post-dispersed, diffraction grating detection system. The challenges of reconstructing astronomical spectra will be reviewed.

© 2018 The Author(s)

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