Cosmic rays from the knee to the highest energies
J Bl�mer, R Engel, JR H�randel�- Progress in Particle and Nuclear Physics, 2009 - Elsevier
This review summarizes recent developments in the understanding of high-energy cosmic
rays. It focuses on galactic and presumably extragalactic particles in the energy range from�…
rays. It focuses on galactic and presumably extragalactic particles in the energy range from�…
Invited review article: IceCube: an instrument for neutrino astronomy
Neutrino astronomy beyond the Sun was first imagined in the late 1950s; by the 1970s, it
was realized that kilometer-scale neutrino detectors were required. The first such instrument�…
was realized that kilometer-scale neutrino detectors were required. The first such instrument�…
Measurement of ultra-high-energy diffuse gamma-ray emission of the Galactic plane from 10 TeV to 1 PeV with LHAASO-KM2A
Z Cao, F Aharonian, Q An, Axikegu, YX Bai, YW Bao…�- Physical Review Letters, 2023 - APS
The diffuse Galactic γ-ray emission, mainly produced via interactions between cosmic rays
and the interstellar medium and/or radiation field, is a very important probe of the�…
and the interstellar medium and/or radiation field, is a very important probe of the�…
The dark matter particle explorer mission
J Chang, G Ambrosi, Q An, R Asfandiyarov…�- Astroparticle�…, 2017 - Elsevier
Abstract The DArk Matter Particle Explorer (DAMPE), one of the four scientific space science
missions within the framework of the Strategic Pioneer Program on Space Science of the�…
missions within the framework of the Strategic Pioneer Program on Space Science of the�…
[HTML][HTML] A deep spectromorphological study of the γ-ray emission surrounding the young massive stellar cluster Westerlund 1
Context. Young massive stellar clusters are extreme environments and potentially provide
the means for efficient particle acceleration. Indeed, they are increasingly considered as�…
the means for efficient particle acceleration. Indeed, they are increasingly considered as�…
A cocoon of freshly accelerated cosmic rays detected by Fermi in the Cygnus superbubble
The origin of Galactic cosmic rays is a century-long puzzle. Indirect evidence points to their
acceleration by supernova shockwaves, but we know little of their escape from the shock�…
acceleration by supernova shockwaves, but we know little of their escape from the shock�…
Closing in on the origin of Galactic cosmic rays using multimessenger information
JB Tjus, L Merten�- Physics Reports, 2020 - Elsevier
In cosmic ray physics extensive progress has been made in recent years, both concerning
theory and observation. The vast details in direct, indirect and secondary detections on the�…
theory and observation. The vast details in direct, indirect and secondary detections on the�…
Sensitivity of the high altitude water Cherenkov detector to sources of multi-TeV gamma rays
AU Abeysekara, R Alfaro, C Alvarez, JD �lvarez…�- Astroparticle�…, 2013 - Elsevier
Abstract The High Altitude Water Cherenkov (HAWC) observatory is an array of large water
Cherenkov detectors sensitive to gamma rays and hadronic cosmic rays in the energy band�…
Cherenkov detectors sensitive to gamma rays and hadronic cosmic rays in the energy band�…
TeV gamma rays from Geminga and the origin of the GeV positron excess
H Y�ksel, MD Kistler, T Stanev�- Physical review letters, 2009 - APS
The Geminga pulsar has long been one of the most intriguing MeV-GeV γ-ray point sources.
We examine the implications of the recent Milagro γ-ray Observatory detection of extended�…
We examine the implications of the recent Milagro γ-ray Observatory detection of extended�…
Milagro observations of multi-TeV emission from Galactic sources in the Fermi bright source list
We present the result of a search of the Milagro sky map for spatial correlations with sources
from a subset of the recent Fermi Bright Source List (BSL). The BSL consists of the 205 most�…
from a subset of the recent Fermi Bright Source List (BSL). The BSL consists of the 205 most�…