Fig. 9
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Cumulative distributions of the median FUV fluxes experienced by discs in the regions selected in ≲200 pc (left panel), Orion (central panel), and Serpens region (right panel). The flux values are the best estimate evaluated using Method 3 (Sect. 4.3). The exception is NGC 2024, where we evaluated the FUV fluxes using Method 2 (Sect. 4.2). We consider them as overestimates of the actual fluxes.
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