Left: position of HD 200775 relative to the NGC 7023 NW filament and footprints of the NIRSpec observations. The background is the F1130W map from the MIRI imager observations of the same program (Misselt et al. 2025). The dashed rectangle indicates the coverage of Spitzer-based spectroscopy and feature maps (Werner et al. 2004; Shannon et al. 2015), which includes coverage closer to the star, where C₆₀ was observed. The labeled footprints are the regions of interest for the studies by Berné & Tielens (2012) and Mackie et al. (2015). The diamond (a 3.6″ square) indicates the typical spectral extraction size for Spitzer-based studies. Right: zoom-in of the same image, showing the two extraction apertures of Misselt et al. (2025) used for the demonstration in Figs. 2 and 3, and the size of a single 0.35″ spaxel of our spectral extractions (Sect. 2). The edge of the mosaic is around 37″ away from the star.