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Fig. 3

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Top: monthly light-curve of FGL J1045.0-5942 derived from the 21-month Fermi/LAT dataset. The red point corresponds to the flux level observed during the X-ray minimum. The black line represent the best result (with its error) obtained assuming a steady flux for the source. Uncertainties are 95% confidence levels. Bottom: residuals from the steady flux fit.

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