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Fig. 1

image

Composite image from BRz Subaru Suprime Cam images of the galaxy NEP J175536.7+664546.8. The thick and thin circles show the positions of the ULX and nearby blobs, respectively, while the size of the circles corresponds to the aperture photometry used for the SED modeling. The rectangle approximately shows the slit geometry utilized in the OSIRIS/GTC spectroscopy.

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