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Fig. 4.
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XMM-Newton 0.2 − 10.0 keV EPICpn light curve of eRO-QPE3, of the first (eRO3-XMM1, left) and second observation (eRO3-XMM2, right). The two eruptions in eRO3-XMM1 are separated by ∼20.4 h. Here, teRO3-XMM1, 0 corresponds to MJD ∼59779.799 and teRO3-XMM2, 0 to ∼59799.745.
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