We present the data reduction software for MIDI written at Sterrewacht Leiden and MPIA Heidelberg. It uses power-spectrum analysis or the information contained in the spectrally-dispersed fringe measurements, in order to estimate the correlated flux and the visibility as function of wavelength in the N-band. © 2007 Springer.
CITATION STYLE
Köhler, R., & Jaffe, W. (2008). MIA+EWS, the software for MIDI data-reduction. In ESO Astrophysics Symposia (Vol. 2008, pp. 569–570). https://doi.org/10.1007/978-3-540-74256-2_93
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