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Fig. 4
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Fermi-LAT 95% upper limits on RS Oph 15 year emission using the template from Healy-Kalesh et al. (2024a) compared with the π0 model. The spectral energy distributions from the outburst period of RS Oph are from Acciari et al. (2022) for the time range shown in the legend, in which RS Oph is assumed to be a point source.
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