Fermi-LAT gamma-ray AGN show higher voidiness than SDSS quasars, explained by line-of-sight interactions boosting flux by about 0.1% per Mpc of void traversed.
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Impacts of Voids, Line of Sight Interactions, and Local Emission Environment on Detectability of Gamma-Ray AGN
Fermi-LAT gamma-ray AGN show higher voidiness than SDSS quasars, explained by line-of-sight interactions boosting flux by about 0.1% per Mpc of void traversed.