[HTML][HTML] “Lomonosov” satellite—space observatory to study extreme phenomena in space

VA Sadovnichii, MI Panasyuk, AM Amelyushkin… - Space Science …, 2017 - Springer
The “Lomonosov” space project is lead by Lomonosov Moscow State University in
collaboration with the following key partners: Joint Institute for Nuclear Research, Russia …

[图书][B] Astroparticle Physics: Theory and Phenomenology

G Sigl - 2017 - Springer
This monograph grew out of a series of lectures and seminars on cosmology, astroparticle
physics and general relativity I have given or co-organized at University of Hamburg and …

Modeling the spectral energy distribution of the radio galaxy IC310

N Fraija, A Marinelli, A Galván-Gámez… - Astroparticle Physics, 2017 - Elsevier
The radio galaxy IC310 located in the Perseus Cluster is one of the brightest objects in the
radio and X-ray bands, and one of the closest active galactic nuclei observed in very-high …

[HTML][HTML] Ultrahigh energy cosmic ray nuclei from remnants of dead quasars

RJ Moncada, RA Colon, JJ Guerra, MJ O'Dowd… - Journal of High Energy …, 2017 - Elsevier
We re-examine the possibility of ultrahigh energy cosmic rays being accelerated in nearby
dormant quasars. We particularize our study to heavy nuclei to accommodate the spectrum …

[PDF][PDF] The observability of jets in cosmic air showers

JMC Montanus - Ph. D. Thesis, 2017 - s3.cern.ch
When a cosmic air shower reaches the detectors at the surface of the earth it can leave a
signal in one or more detectors. The core of the shower has to be determined out of the …

The current status of research in ultrahigh-energy cosmic ray physics: A brief review

MY Zotov, OE Kalashev, MS Pshirkov - Moscow University Physics …, 2017 - Springer
The origin and nature of ultrahigh-energy cosmic rays (UHECRs, E> 10 18 eV) is one of the
most intriguing unsolved problems of modern astrophysics. This review is dedicated to the …

Características de la producción científica de instituciones de Puebla indexada en la Web of Science

AF Díaz-Cárdenas, MR Sankey-García… - Investigación …, 2017 - scielo.org.mx
En este artículo describimos el ámbito de la investigación en el estado de Puebla, México,
cuyos resultados han sido publicados en revistas indizadas en la Web of Science (WoS). El …

[PDF][PDF] Anisotropy and chemical composition of ultra-high energy cosmic rays using arrival directions measured by the Pierre Auger...

KSC Mora, M Melissas, F Montanet, JR Martino - academia.edu
Anisotropy and composition, together with the study of the features in the energy spectrum,
are the fundamental tools available to decipher the origin and nature of the ultra-high energy …

[PDF][PDF] Cross correlation of UHECRs and local matter distribution taking into account the energy attenuation due to interaction with the cosmic background radiation

CSL Pintoa, V Bragab, RM de Almeidaa… - inspirehep.net
The arrival direction distribution of ultra-high energy cosmic rays (UHECRs, particles with
energy exceeding E> 1019 eV) is an important observable to understand the origin and …

A Bayesian on–off analysis of cosmic ray data

D Nosek, J Nosková - Nuclear Instruments and Methods in Physics …, 2017 - Elsevier
We deal with the analysis of on–off measurements designed for the confirmation of a weak
source of events whose presence is hypothesized, based on former observations. The …