Searches for correlation between UHECR events and high-energy gamma-ray Fermi-LAT data
arXiv:1611.09869 · doi:10.1088/1475-7516/2016/12/023
Abstract
The astrophysical sources responsible for ultra high-energy cosmic rays (UHECRs) continue to be one of the most intriguing mysteries in astrophysics. We present a comprehensive search for correlations between high-energy ( GeV) gamma-ray events from the Fermi Large Area Telescope (LAT) and UHECRs ( EeV) detected by the Telescope Array and the Pierre Auger Observatory. We perform two separate searches. First, we conduct a standard cross-correlation analysis between the arrival directions of 148 UHECRs and 360 gamma-ray sources in the Second Catalog of Hard Fermi-LAT sources (2FHL). Second, we search for a possible correlation between UHECR directions and unresolved Fermi-LAT gamma-ray emission. For the latter, we use three different methods: a stacking technique with both a model-dependent and model-independent background estimate, and a cross-correlation function analysis. We also test for statistically significant excesses in gamma rays from signal regions centered on Cen A and the Telescope Array hotspot. No significant correlation is found in any of the analyses performed, except a weak () hint of signal with the correlation function method on scales . Upper limits on the flux of possible power-law gamma-ray sources of UHECRs are derived.
24 pages, 12 figures, accepted in JCAP
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