A Study on the Line of Sight to Galaxies Detected at Gamma-Ray Energies

Abstract

The large-scale universal structure comprises strands of dark matter and galaxies with large underdense volumes known as voids. We measure the fraction of the line of sight that intersects voids for active galactic nuclei (AGN) detected by Fermi Large Area Telescope (LAT) and quasars from the Sloan Digital Sky Survey (SDSS). This “voidiness” fraction is a rudimentary proxy for the density along the line of sight to the galaxies. The voidiness of SDSS-observed quasars (QSOs) is distinctly different from randomly distributed source populations, with a median p -value of 4.6 × 10 ^−5 and ≪1 × 10 ^−7 , when compared with 500 simulated populations with randomly simulated locations but matching redshifts in the 0.1 ≤ z 0.05). We do not study possible causes of this voidiness difference. It might relate to propagation effects from lower magnetic or radiative background fields within voids or to an environment more favorable for gamma-ray production for AGN near voids.

Keywords

• Gamma-rays
• Blazars
• Voids
• Gamma-ray sources
• Gamma-ray astronomy