Fig. 1.
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X-ray image of NGC 1566 (in center), accumulated by /XRT from December 12, 2007 to November 2, 2023 with a 230 ks exposure time. The yellow contours in this image demonstrate the lack of X-ray jet-like structure, as well as minimal contamination by other point sources within 18″. The closest next source is 21″(LSXPS J041956.5–545528 is marked with a green circle).
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