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Fig. 1

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a) Periodogram of Swift-BAT (15–50 keV) data for IGR J05007−7047. b) Distribution of values excluding the intervals around Po and its multiples. The continuous line is the best fit obtained with an exponential model applied to the tail of the distribution (χ2 > 15). c) Swift-BAT light curve folded at P = 30.77 ± 0.01 d period in 16 phase bins.

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