Fig. 13
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Comparison of 0.2–2.3 keV flux distributions of eRO-ExTra with those of variable or transient extragalactic sources in previous studies. The dashed red line shows this study, the orange line shows XMM-COSMOS (Lanzuisi et al. 2014), the dotted black line shows eRASS1 (Boller et al. 2024), and the dashed blue line shows ROSAT (Fuhrmeister & Schmitt 2003).
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