… We present measurements of the large-scale cosmic-ray (CR) anisotropies in RA, using data
collected by the surface detector array of the Pierre Auger Observatory over more than 14 yr.
We determine the equatorial dipole component, ${{\boldsymbol{d}}}_{\perp }$ … More precise
measurements of the large-scale anisotropies, filling the gap between the IceCube/IceTop or
KASCADE-Grande measurements and the dipole determined by the Pierre Auger Observatory
above 8 EeV, should provide information about this transition. In fact, although at energies …

Agradecimentos: The successful installation, commissioning, and operation of the Pierre
Auger Observatory would not have been possible without the strong commitment and effort
from the technical and administrative staff in Malargüe. We are very grateful to the following
agencies and organizations for financial support: Argentina—Comisión Nacional de Energía
Atómica; Agencia Nacional de Promoción Científica y Tecnológica (ANPCyT); Consejo
Nacional de Investigaciones Científicas y Técnicas (CONICET); Gobierno de la Provincia de …