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View article: Delayed cutaneous wound healing in young and old female mice is associated with differential growth factor release but not inflammatory cytokine secretion
Delayed cutaneous wound healing in young and old female mice is associated with differential growth factor release but not inflammatory cytokine secretion Open
The capacity for tissue repair during wound healing declines with age. A chronic low but systemic inflammatory status, often called “inflammaging”, is considered a key factor that contributes to impaired tissue regeneration. This phenomeno…
View article: A multi-detector EAS reconstruction framework for IceCube
A multi-detector EAS reconstruction framework for IceCube Open
The IceCube Neutrino Observatory is also a very unique extensive air shower (EAS) detector, that simultaneously measures the EAS footprint on the surface and the high-energy muons in deep ice. The surface array - IceTop, comprising of ice-…
View article: Snowmass UHECR Whitepaper: Requirements on Future Instrumentation
Snowmass UHECR Whitepaper: Requirements on Future Instrumentation Open
Complementing the overview contribution about the whitepaper on ultra-high-energy cosmic rays (UHECR) prepared for the Snowmass community survey in the U.S. [Astroparticle Physics 149 (2023) 102819 - arXiv:2205.05845], this contribution fo…
View article: “Ultra-High-Energy Cosmic-Rays (UHECR): at the Intersection of the Cosmic and Energy Frontiers” -- Overview of the Snowmass UHECR white paper and roadmap
“Ultra-High-Energy Cosmic-Rays (UHECR): at the Intersection of the Cosmic and Energy Frontiers” -- Overview of the Snowmass UHECR white paper and roadmap Open
As part of the US "Snowmass" community planning exercise, the UHECR community has come together to write a comprehensive white paper discussing the recent progress and open questions of the field, as they relate to the overarching goals of…
View article: Measurements of Cosmic Ray Mass Composition with the IceCube Neutrino Observatory
Measurements of Cosmic Ray Mass Composition with the IceCube Neutrino Observatory Open
The IceCube Neutrino Observatory is a multi-component detector at the South Pole. Besides studying high-energy neutrinos, it is capable of measuring high-energy cosmic rays from PeV to EeV. This energy region is thought to cover the transi…
View article: Hybrid cosmic ray measurements using the IceAct telescopes in coincidence with the IceCube and IceTop detectors
Hybrid cosmic ray measurements using the IceAct telescopes in coincidence with the IceCube and IceTop detectors Open
IceAct is a proposed surface array of compact (50 cm diameter) and cost-effective Imaging Air Cherenkov Telescopes installed at the site of the IceCube Neutrino Observatory at the geographic South Pole. Since January 2019, two IceAct teles…
View article: Hybrid cosmic ray measurements using the IceAct telescopes in\n coincidence with the IceCube and IceTop detectors
Hybrid cosmic ray measurements using the IceAct telescopes in\n coincidence with the IceCube and IceTop detectors Open
IceAct is a proposed surface array of compact (50 cm diameter) and\ncost-effective Imaging Air Cherenkov Telescopes installed at the site of the\nIceCube Neutrino Observatory at the geographic South Pole. Since January 2019,\ntwo IceAct te…
View article: Simulation and Reconstruction Study of a Future Surface Scintillator Array at the IceCube Neutrino Observatory
Simulation and Reconstruction Study of a Future Surface Scintillator Array at the IceCube Neutrino Observatory Open
The IceCube Neutrino Observatory at the South Pole is a multi-component particle detector consisting of the IceTop surface array and the deep in-ice IceCube array. The foreseen enhancement of the surface instrumentation will consist of pla…
View article: Cosmic Ray Spectrum and Composition from PeV to EeV from the IceCube\n Neutrino Observatory
Cosmic Ray Spectrum and Composition from PeV to EeV from the IceCube\n Neutrino Observatory Open
The IceCube Neutrino Observatory at the South Pole is a multi-component\ndetector capable of measuring the cosmic ray energy spectrum and composition\nfrom PeV to EeV, the energy region typically thought to cover the transition\nfrom galac…
View article: Cosmic Ray Spectrum and Composition from PeV to EeV from the IceCube Neutrino Observatory
Cosmic Ray Spectrum and Composition from PeV to EeV from the IceCube Neutrino Observatory Open
The IceCube Neutrino Observatory at the South Pole is a multi-component detector capable of measuring the cosmic ray energy spectrum and composition from PeV to EeV, the energy region typically thought to cover the transition from galactic…
View article: Cosmic ray composition study using machine learning at the IceCube Neutrino Observatory
Cosmic ray composition study using machine learning at the IceCube Neutrino Observatory Open
The evaluation of mass composition of cosmic rays in the knee region (~3 PeV) is critical to understanding the transition in the origin of cosmic rays from galactic to extragalactic sources. The IceCube Neutrino Observatory at the South Po…
View article: Cosmic ray composition study using machine learning at the IceCube\n Neutrino Observatory
Cosmic ray composition study using machine learning at the IceCube\n Neutrino Observatory Open
The evaluation of mass composition of cosmic rays in the knee region ($\\sim\n3$ PeV) is critical to understanding the transition in the origin of cosmic\nrays from galactic to extragalactic sources. The IceCube Neutrino Observatory\nat th…
View article: Cosmic ray composition study using machine learning at the IceCube Neutrino Observatory
Cosmic ray composition study using machine learning at the IceCube Neutrino Observatory Open
The evaluation of mass composition of cosmic rays in the knee region ($\sim 3$ PeV) is critical to understanding the transition in the origin of cosmic rays from galactic to extragalactic sources. The IceCube Neutrino Observatory at the So…
View article: Cosmic Ray Spectrum and Composition from PeV to EeV from the IceCube Neutrino Observatory
Cosmic Ray Spectrum and Composition from PeV to EeV from the IceCube Neutrino Observatory Open
The IceCube Neutrino Observatory at the South Pole is a multi-component detector capable of measuring the cosmic ray energy spectrum and composition from PeV to EeV, the energy region typically thought to cover the transition from galactic…
View article: Latest Cosmic Ray Results from IceTop and IceCube
Latest Cosmic Ray Results from IceTop and IceCube Open
The IceCube Neutrino Observatory at the geographic South Pole, with its surface array IceTop, detects three different components of extensive air showers: the total signal at the surface, low energy muons on the periphery of the showers, a…
View article: Measurements of the Mass Composition of UHECRs with the Pierre Auger Observatory
Measurements of the Mass Composition of UHECRs with the Pierre Auger Observatory Open
As a hybrid cosmic ray detector, the Pierre Auger Observatory can measure the longitudinal air shower development with the fluorescence detector, and the lateral distribution of particles reaching the ground with the surface detector.We re…
View article: Measurement of the chemical composition of ultra high energy cosmic rays with the HEAT telescopes of the Pierre Auger Observatory
Measurement of the chemical composition of ultra high energy cosmic rays with the HEAT telescopes of the Pierre Auger Observatory Open
The Pierre Auger Observatory is currently the largest detector for measurements of cosmic rays with energies beyond 10^18 eV. It uses a hybrid detection method with fluorescence telescopes and surface detector stations. Cosmic rays with en…
View article: Measurement of the chemical composition of the ultra-high-energy cosmic rays with the Pierre Auger Observatory
Measurement of the chemical composition of the ultra-high-energy cosmic rays with the Pierre Auger Observatory Open
The Pierre Auger Observatory infers the chemical composition of ultra-high-energy cosmic rays through two independent detection techniques. The Fluorescence Detector (FD) measures the longitudinal profile of high energy air showers and can…
View article: Measurement of the chemical composition of the ultra-high-energy cosmic\n rays with the Pierre Auger Observatory
Measurement of the chemical composition of the ultra-high-energy cosmic\n rays with the Pierre Auger Observatory Open
The Pierre Auger Observatory infers the chemical composition of\nultra-high-energy cosmic rays through two independent detection techniques. The\nFluorescence Detector (FD) measures the longitudinal profile of high energy air\nshowers and …
View article: Search for patterns by combining cosmic-ray energy and arrival directions at the Pierre Auger Observatory
Search for patterns by combining cosmic-ray energy and arrival directions at the Pierre Auger Observatory Open
Energy-dependent patterns in the arrival directions of cosmic rays are searched for using data of the Pierre Auger Observatory. We investigate local regions around the highest-energy cosmic rays with E > = 6×1019 eV by analyzing cosmic ray…