Oxford University Press (OUP), Monthly Notices of the Royal Astronomical Society, 1(440), p. 161-171
DOI: 10.1093/mnras/stu133
Full text: Download
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 10–25 kpc, in the region of the sky approximately bounded by 30 ◦