Systematic evaluation of variability detection methods for eROSITA

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

Open Access

Fig. 1

Example counts of the tenth brightest eFEDS source. The markers indicate the number of counts from a single eROSITA telescope module in 100s time bins, recorded over a six-hour period. The black curve shows the sensitivity to the source position over time.

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