Optimisation-based alignment of wide-band integrated superconducting spectrometers for submillimeter astronomy

Open Access

Fig. 6

2D sketch of the warm focal plane and the parameters described in Eq. (4). The figure is a zoom of the warm focal plane shown in Fig. 2. The misaligned-ray direction is exaggerated. The coordinate system is identical to the system shown in Fig. 1a.

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