Indication of Gamma-Ray Emission from the Newly Discovered Dwarf Galaxy Reticulum II

We present a search for γ -ray emission from the direction of the newly discovered dwarf galaxy Reticulum II. Using Fermi-LAT Collaboration data, we detect a signal that exceeds expected backgrounds between ∼2 - 10 GeV and is consistent with annihilation of dark matter for particle masses less than a few ×1 0² GeV . Modeling the background as a Poisson process based on Fermi-LAT diffuse models, and taking into account trial factors, we detect emission with p value less than 9.8 ×1 0^-5 (>3.7 σ ). An alternative, model-independent treatment of the background reduces the significance, raising the p value to 9.7 ×1 0^-3 (2.3 σ ). Even in this case, however, Reticulum II has the most significant γ -ray signal of any known dwarf galaxy. If Reticulum II has a dark-matter halo that is similar to those inferred for other nearby dwarfs, the signal is consistent with the s -wave relic abundance cross section for annihilation.