22–25 Jan 2019
Padova
Europe/Rome timezone

Ultra-high energy cosmic ray anisotropies measured with the Pierre Auger Observatory

24 Jan 2019, 15:20
20m
Polo di Psicologia - room 3I (3rd floor, building 2) (Padova)

Polo di Psicologia - room 3I (3rd floor, building 2)

Padova

Via Venezia, 12-14 Padova
Talk Main track Connection to UHECR

Speaker

Prof. Guenter Sigl (Universität Hamburg)

Description

Recently the Pierre Auger Observatory has observed a dipolar anisotropy of amplitude ~ 6.5% above 8 x 10^{18} eV that is unrelated to the Galactic plane. While the significance is largest above 8 x 10^{18} eV, the cosmic-ray data indicate a growth of the dipolar amplitude from 4 to 32 EeV and beyond. Furthermore, above 4 x 10^{19} eV, indications have been found for intermediate-scale anisotropies associated with extragalactic gamma-ray sources. Apart from those indications no significant anisotropies are seen. We review these observations and discuss possible astrophysical interpretations, in particular in the context of the sources discussed at this conference.

Are you presenting on behalf of collaborations or institutions?

on behalf of the Pierre Auger collaboration

Primary author

Prof. Guenter Sigl (Universität Hamburg)

Presentation materials