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20092026
most citedThe First LHAASO Catalog of Gamma-Ray Sources

247 citations · 2.6k across the 118 of their papers we have counts for

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Showing 2011Show all

6 papers · 1 filter

astro-ph.HE2011★ 95 cited

Cosmic Ray Anisotropy as Signature for the Transition from Galactic to Extragalactic Cosmic Rays

G. Giacinti, M. Kachelriess, D. V. Semikoz +1

We constrain the energy at which the transition from Galactic to extragalactic cosmic rays occurs by computing the anisotropy at Earth of cosmic rays emitted by Galactic sources. S…

astro-ph.HE2011★ 110 cited

Local Magnetic Turbulence and TeV-PeV Cosmic Ray Anisotropies

G. Giacinti, G. Sigl

In the energy range from ~ 10^12 eV to ~ 10^15 eV, the Galactic cosmic ray flux has anisotropies both on large scales, with an amplitude of the order of 0.1%, and on scales between…

astro-ph.HE2011

Propagation of Ultrahigh Energy Nuclei in the Magnetic Field of our Galaxy

G. Giacinti, M. Kachelriess, D. V. Semikoz +1

In this work, we present detailed simulations for propagation of ultra-high energy (UHE) heavy nuclei, with E > 60 EeV, within recent Galactic Magnetic Field (GMF) models. We inves…

astro-ph.HE2011

Search for Nuclei Sources in the Ultra-High Energy Cosmic Ray Data

G. Giacinti, D. V. Semikoz

We present a new method to search for heavy nuclei sources, on top of background, in the Ultra-High Energy Cosmic Ray data. We apply it to the 69 events with energies E>55 EeV publ…

astro-ph.HE2011

Search for Individual Ultrahigh Energy Cosmic Ray Sources in the Future Data

G. Giacinti, D. V. Semikoz

We propose a new way to detect individual bright Ultra-High Energy Cosmic Ray (UHECR) sources above background if the Galactic Magnetic Field (GMF) gives the main contribution to U…

astro-ph.HE2011★ 51 cited

Ultrahigh Energy Nuclei in the Turbulent Galactic Magnetic Field

G. Giacinti, M. Kachelriess, D. V. Semikoz +1

In this work we study how the turbulent component of the Galactic magnetic field (GMF) affects the propagation of ultrahigh energy heavy nuclei. We investigate first how the images…