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. 22

Variability of SXP 726 as observed by XMM-Newton and eROSITA (red). The blue points correspond to flux values reported by Eger & Haberl (2008b), whereas black points are reported here for the first time. The upper limits for observations when the source was not detected are also indicated (green arrows).

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