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Fig. A.1
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Images of eROSITA eRASS1 0.2-2.3 keV (left) and 2MASS K (right) overlaid with X-ray contours of IRAS 02346-6248 (also known as RS Hor). The contours have been derived from a resampled and Gaussian-smoothed X-ray image with levels at 30%, 50%, 70%, and 90% of the count peak in the central 2′ × 2′ region.
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