2014MNRAS.440..161S

We map the large-scale sub-structure in the Galactic stellar halo using accurate 3D positions of ∼ 14 000 RR Lyrae reported by the Catalina Sky Survey. In the heliocentric distance range of 10^–25kpc, in the region of the sky approximately bounded by 30° < l < 55° and -45° < b < -25°, there appears to be a strong excess of RRab stars. This overdensity, peaking at 18kpc, is most likely associated with the so-called Hercules-Aquila Cloud (HAC), previously detected using main-sequence tracers at similar distances in the Sloan Digital Sky Survey data. Our analysis of the period-amplitude distribution of RR Lyrae in this region indicates that the HAC is dominated by the Oosterhoff I type population. By comparing the measured RR Lyrae number density to models of a smooth stellar halo, we estimate the significance of the observed excess and provide an updated estimate of the total luminosity of the Cloud's progenitor.