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Fig. 6

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Flux time history of 2FGL J1045.0−5941 as determined by likelihood analysis for ranges of the orbital phase of η Car (left) and the physical separation of the stellar components (right) for energies 10 to 300 GeV. Each data point represents five months of data. Because periastron is traversed very quickly, the data points around orbital phase 0 are very broad. The region between the two dashes at the left of the horizontal error bar of the second data point on the right graph is traversed twice.

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