The ultra-high energy cosmic rays image of Virgo A

Radio Detection of Horizontal Extensive Air Showers with AERA

Results from Pion-Carbon Interactions Measured by NA61/SHINE for Improved Understanding of Extensive Air Showers

Detecting particles with cell phones: the Distributed Electronic Cosmic-ray Observatory

Infinite efficiency of collisional Penrose process: Can over-spinning Kerr geometry be the source of ultra-high-energy cosmic rays and neutrinos?

The origin of IceCube's neutrinos: Cosmic ray accelerators embedded in star forming calorimeters

Luminosity of ultrahigh energy cosmic rays and bounds on magnetic luminosity of radio-loud active galactic nuclei

Pierre Auger Observatory and Telescope Array: Joint Contributions to the 34th International Cosmic Ray Conference (ICRC 2015)

The IceCube Neutrino Observatory, the Pierre Auger Observatory and the Telescope Array: Joint Contribution to the 34th International Cosmic Ray Conference (ICRC 2015)

Cosmic ray transport and anisotropies to high energies

Sensitivity of the JEM-EUSO telescope to gravity effects in neutrino-induced air showers

IceCube Constraints on Fast-Spinning Pulsars as High-Energy Neutrino Sources

The Galactic magnetic field and its lensing of ultrahigh energy and Galactic cosmic rays

Origin of the ankle in the ultra-high energy cosmic ray spectrum and of the extragalactic protons below it

A Uniformly Selected, All-Sky Optical AGN catalog, for UHECR Correlation

Surprises from extragalactic propagation of UHECRs

Extreme BL Lacs: probes for cosmology and UHECR candidates

Ultra-high-energy-cosmic-ray hot spots from tidal disruption events

Maximum entropy analysis of cosmic ray composition

We focus on the primary composition of cosmic rays with the highest energies that cause extensive air showers in the Earth's atmosphere. A way of examining the two lowest order moments of the sample distribution of the depth of shower maximum is presented. The aim is to show that useful information about the composition of the primary beam can be inferred with limited knowledge we have about processes underlying these observations. In order to describe how the moments of the depth of shower maximum depend on the type of primary particles and their energies, we utilize a superposition model. Using the principle of maximum entropy, we are able to determine what trends in the primary composition are consistent with the input data, while relying on a limited amount of information from shower physics. Some capabilities and limitations of the proposed method are discussed. In order to achieve a realistic description of the primary mass composition, we pay special attention to the choice of the parameters of the superposition model. We present two examples that demonstrate what consequences can be drawn for energy dependent changes in the primary composition.

[arXiv:1512.09248]

Molecular Bremsstrahlung Radiation at GHz Frequencies in Air

Radio detection of high-energy cosmic rays with the Auger Engineering Radio Array (PISA 2015)

A Bayesian analysis of the 69 highest energy cosmic rays detected by the Pierre Auger Observatory

The sensitivity of past and near-future lunar radio experiments to ultra-high-energy cosmic rays and neutrinos

Proposal of the Electrically Charged Stellar Black Holes as Accelerators of Ultra High Energy Cosmic Rays

Ultrahigh-Energy Cosmic Rays from the "En Caul" Birth of Magnetars

Constraining pion interactions at very high energies by cosmic ray data

An All-Sky Search for Three Flavors of Neutrinos from Gamma-Ray Bursts with the IceCube Neutrino Observatory

Detection prospects of the TA hotspot by space observatories

The Influence of Magnetic Fields on UHECR Propagation from Virgo A

Energy and flux measurements of ultra-high energy cosmic rays observed during the first ANITA flight

Ultrahigh Energy Cosmic Rays and Black Hole Mergers

Evidence for a Local "Fog" of Sub-Ankle UHECR

On ultra high energy cosmic rays and their resultant gamma rays

First Upper Limits on the Radar Cross Section of Cosmic-Ray Induced Extensive Air Showers

Characteristics of Four Upward-pointing Cosmic-ray-like Events Observed with ANITA

Ultra High Energy Cosmic Rays and Neutrinos

CRPropa 3 - a Public Astrophysical Simulation Framework for Propagating Extraterrestrial Ultra-High Energy Particles

High energy electromagnetic cascades in extragalactic space: physics and features

Azimuthal asymmetry in the risetime of the surface detector signals of the Pierre Auger Observatory

Ultrahigh Energy Cosmic Rays: A Galactic Origin?

Measurement of the Radiation Energy in the Radio Signal of Extensive Air Showers as a Universal Estimator of Cosmic-Ray Energy

New Limits on Extragalactic Magnetic Fields from Rotation Measures

Uncertainty from Extrapolation of Cosmic Ray Air Shower Parameters

Evidence that the maximum electron energy in hotspots of FR II galaxies is not determined by synchrotron cooling

Multi-PeV Signals from a New Astrophysical Neutrino Flux Beyond the Glashow Resonance

Sensitivity of the space-based CHerenkov from Astrophysical Neutrinos Telescope (CHANT)

Neutrino, γ-ray and cosmic ray fluxes from the core of the closest radio galaxies

Constraints on ultra-high-energy cosmic ray sources from a search for neutrinos above 10 PeV with IceCube

Nuclear Physics Meets the Sources of the Ultra-High Energy Cosmic Rays

Radio detection of Cosmic-Ray Air Showers and High-Energy Neutrinos

Propagation of Ultra High Energy Cosmic Rays in Extragalactic Magnetic Fields: A view from cosmological simulations

A roadmap for searching cosmic rays correlated with the extraterrestrial neutrinos seen at IceCube

Results and Perspectives of the Auger Engineering Radio Array

Measurement of the Muon Production Depths at the Pierre Auger Observatory

Cosmogenic photons strongly constrain UHECR source models

Air Shower Radio Emission with Energy E0≥1019 eV by Yakutsk Array Data

LIC and LID considerations in the design and implementation of the MEMS laser pointing mechanism for the EUSO UV laser altimeter

The Nature and Origin of Ultra-High Energy Cosmic Ray Particles

Cosmic ray composition measurements and cosmic ray background free gamma-ray observations with Cherenkov telescopes

A new method to test the hypothesis of isotropy of the ultrahigh energy cosmic ray flux

A study of photons at ultra high energy using Auger surface detector

Международная конференция по космическим лучам

Международная конференция по космическим лучам пройдет с 12 по 20 июля 2017 года в городе Пусан (Южная Корея).

Подробная информация на сайте конференции:

http://icrc2017.org/

The JEM-EUSO program

Extended European Cosmic Ray Symposium (E+CRS 2018)