eROSITA calibration and performance verification phase: High-mass X-ray binaries in the Magellanic Clouds

The Early Data Release of eROSITA and Mikhail Pavlinsky ART-XC on the SRG mission

Open Access

Fig. 3

eROSITA colour image (red: 0.2–1.0 keV, green: 1.0–2.0keV, and blue: 2.0–4.5 keV) of the region around SRGEt J052829.5–690345. The transient source appears similar in colours to the SFXT XMMUJ053108.3–690923 (Maitra et al. 2021), which is located at an angular distance of~15′. The soft extended X-ray emission from the supernova remnant MCSNR J0527–6912 (e.g. Maggi et al. 2016) is also marked.

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