Reply to "Comment on `Correlation between Compact Radio Quasars and Ultra-High Energy Cosmic Rays'"
arXiv:astro-ph/9901315 · doi:10.1103/PhysRevLett.83.2472
Abstract
We discuss the rationale for the energy cuts used in the previous study of directional correlation of the five highest energy cosmic ray events with compact, radio quasars. We check the consistency of the next three most energetic events which just missed those cuts, with the correlation hypothesis. Agreement between expected and observed properties of these events is good.
2 pp revtex
References in corpus (3)
Cited by in corpus (15)
- Origin and Propagation of Extremely High Energy Cosmic Rays
- Compact steep-spectrum and peaked-spectrum radio sources
- Ultra-High Energy Neutrino Fluxes and Their Constraints
- The high energy cosmic ray spectrum from relic particle decay
- Astrophysical Origins of Ultrahigh Energy Cosmic Rays
- Ultrahigh Energy Cosmic Rays: The state of the art before the Auger Observatory
- Ultra-High Energy Cosmic Rays from Neutrino Emitting Acceleration Sources?
- Ultra-High Energy Cosmic Rays: A Probe of Physics and Astrophysics at Extreme Energies
- Testing the Correlation of Ultra-High Energy Cosmic Rays with High Redshift Sources
- The clustering of ultra-high energy cosmic rays and their sources
- Axion-like particles as ultra high energy cosmic rays?
- On the cross correlation between the arrival direction of ultra-high energy cosmic rays, BL Lacertae, and EGRET detections: A new way to identify EGRET sources?
- Footprints of Super-GZK Cosmic Rays in the Pilliga State Forest
- Constraints on ultra-high energy neutrinos from optically thick astrophysical accelerators
- Ultra high energy cosmic ray sources & experimental results