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Fig. 2


4 h average light curves in counts per second of the persistent emission of GS 0836–429 built from data collected by JEM-X (3.5–25 keV, upper panel) and IBIS/ISGRI (17–80 keV, lower panel). The red arrows and the blue arrows shown in the upper panel indicate the time when the normal Type I X-ray bursts and the SWT bursts respectively occurred (57, see Table 1).

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