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)
PDF ArticleMore Like This
David Naylor, Brad Gom, Ian Veenendaal, Dennis van Loon, Willem Jellema, Peter Roelfsema, Kees Wafelbakker, Alain Cournoyer, and Frederic Grandmont
FW3B.1 Fourier Transform Spectroscopy (FTS) 2018
David Naylor, Peter Roelfsema, Martin Giard, Francisco Najarro, Kees Wafelbakker, Willem Jellema, Brian Jackson, Bruce Swinyard, Marc Audard, Yasuo Doi, Matt Griffin, Frank Helmich, Franz Kerschbaum, Michael Meyer, Hans Nielsen, Göran Olofsson, Albrecht Poglitsch, Luigi Spinoglio, Bart Vandenbussche, Kate Isaak, and Javier R. Goicoechea
FM4D.2 Fourier Transform Spectroscopy (FTS) 2013
Willem Jellema, David A. Naylor, and Peter Roelfsema
FM2D.6 Fourier Transform Spectroscopy (FTS) 2016