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A New Model of the Galactic Magnetic Field
- R. Jansson, G. Farrar
- Physics
- 16 April 2012
A new, much-improved model of the Galactic magnetic field (GMF) is presented. We use the WMAP7 Galactic synchrotron emission map and more than 40,000 extragalactic rotation measures to constrain the…
The Pierre Auger Collaboration
- M. Will, L. Wiencke, M. Ziolkowski
- Physics
- 1 June 2013
The Pierre Auger Collaboration has reported evidence for anisotropies in the arrival directions of cosmic rays with energies larger thanEth = 55 EeV. There is a correlation above the isotropic…
The 2dF Galaxy Redshift Survey: Luminosity functions by density environment and galaxy type
We use the 2dF Galaxy Redshift Survey to measure the dependence of the bJ-band galaxy luminosity function on large-scale environment, defined by density contrast in spheres of radius 8h-1 Mpc, and on…
The speed of the ‘bullet’ in the merging galaxy cluster 1E0657−56
- V. Springel, G. Farrar
- Physics
- 12 March 2007
Deep Chandra exposures of the hot galaxy cluster 1E0657-56 have revealed a highly dynamical state of the system due to an ongoing merger with a massive subcluster. The system is observed shortly…
The Pierre Auger Cosmic Ray Observatory
- A. Aab, P. Abreu, F. Zuccarello
- Physics
- 21 October 2015
Correlation of the highest energy cosmic rays with nearby extragalactic objects
- J. Abraham, P. Abreu, M. Ziolkowski
- Physics
- 9 November 2007
Using data collected at the Pierre Auger Observatory during the past 3.7 years, we demonstrate that there is a correlation between the arrival directions of cosmic rays with energy above {approx} 6 x…
Correlation of the highest-energy cosmic rays with the positions of nearby active galactic nuclei
- J. Abraham, P. Abreu, M. Ziolkowski
- Physics
- 1 April 2008
Correlation of the highest-energy cosmic rays with nearby extragalactic objects.
- J. Abraham, P. Abreu, B. Kégl
- PhysicsScience
- 26 November 2007
Using data collected at the Pierre Auger Observatory during the past 3.7 years, we demonstrated a correlation between the arrival directions of cosmic rays with energy above 6 x 10(19) electron volts…
Observation of a large-scale anisotropy in the arrival directions of cosmic rays above 8 × 1018 eV
- A. Aab, P. Abreu, F. Zuccarello
- PhysicsScience
- 21 September 2017
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