Simulating the Retrieval of Astronomical Spectra from the SPICA SAFARI Post Dispersed Fourier Transform Spectrometer
2018
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.
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