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The recent detection of γ‐ray emission from four radio‐loud narrow‐line Seyfert 1 galaxies suggests that the engine driving the active galactic nuclei (AGN) activity of these objects shares some similarities with that of blazars, namely the presence of a γ‐ray emitting, variable jet of plasma closely aligned to the line of sight. In this work we analyse the γ‐ray light curves of the four radio‐loud...
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