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Analysis of 42 Years of Cosmic Ray Measurements by the Neutron Monitor at Lomnický štít Observatory
Published 2025-01-01“…Our investigation is centered on the relationships among the solar radio flux, geomagnetic field activity, and cosmic ray flux, as observed by the Neutron Monitor at the Lomnický štít Observatory in Slovakia. …”
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Large-scale Cosmic-ray Anisotropies with 19 yr of Data from the Pierre Auger Observatory
Published 2024-01-01“…Results are presented for the measurement of large-scale anisotropies in the arrival directions of ultra–high-energy cosmic rays detected at the Pierre Auger Observatory during 19 yr of operation, prior to AugerPrime, the upgrade of the observatory. …”
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Prospects for Gamma-Ray Emission from Magnetar Regions in CTAO Observations
Published 2025-01-01Subjects: Get full text
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Ultra-High-Energy Cosmic Rays Accelerated by Magnetically Dominated Turbulence
Published 2024-01-01“…Ultra-high-energy cosmic rays (UHECRs), particles characterized by energies exceeding 10 ^18 eV, are generally believed to be accelerated electromagnetically in high-energy astrophysical sources. …”
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Ultra high energy cosmic rays versus models of high energy hadronic interactions
Published 2025-02-01“…To mitigate possible systematic biases, we include all primaries up to iron, compensate for the differences between the measured and simulated energy spectra of cosmic rays and account for other known systematic effects. …”
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Radio Detection of UHE Cosmic Rays and Neutrinos off the Moon with Two 30 m Telescopes
Published 2024-12-01Get full text
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Contribution of Unresolved Sources to Diffuse Gamma-Ray Emission from the Galactic Plane
Published 2025-01-01“…The diffuse gamma-ray emission from the Milky Way serves as a crucial probe for understanding the propagation and interactions of cosmic rays within our Galaxy. …”
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The Disk Wind Contribution to the Gamma-Ray Emission from the Nearby Seyfert Galaxy GRS 1734−292
Published 2025-01-01“…Such a detection would substantially improve our understanding of cosmic-ray acceleration efficiency in AGN disk wind systems and would establish radio-quiet Seyfert galaxies as cosmic-ray accelerators capable of reaching ultrahigh energies.…”
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Search for Neutrino Signals Correlated with LHAASO Diffuse Galactic Emission
Published 2025-01-01“…The diffuse Galactic γ -ray emission originates from the interactions between cosmic rays and the interstellar medium or radiation fields within our Galaxy, where the production of neutrinos is also anticipated. …”
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The Pierre Auger Observatory open data
Published 2025-01-01“…In February 2021, a portal was released containing 10% of cosmic-ray data collected by the Pierre Auger Observatory from 2004 to 2018, during the first phase of operation of the Observatory. …”
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Solar Modulation of AMS-02 Daily Proton and Helium Fluxes with Modified Force-field Approximation Models
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Recent Data of Extensive Air Showers Recorded by Alborz I Array and Their Detailed Analysis
Published 2022-10-01Get full text
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Study on Test‐Mass Charging for Taiji Gravitational Wave Observatory
Published 2024-01-01“…This study aims to model the charging of TMs during Galactic cosmic rays and solar proton events (SPEs) using the Monte Carlo simulation toolkit meanwhile with constructing the sophisticated 3D spacecraft. …”
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The Cosmic History of Black Hole Growth from Deep Multiwavelength Surveys
Published 2012-01-01“…In this paper, we begin by reviewing the spectral signatures of active galactic nuclei (AGN) ranging from radio to hard X-ray wavelengths. We then describe the most commonly used methods to find these sources, including optical/UV, radio, infrared, and X-ray emission, and optical emission lines. …”
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COSMIC: A Galaxy Cluster–Finding Algorithm Using Machine Learning
Published 2025-01-01Get full text
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MAMMOTH-Subaru. II. Diverse Populations of Circumgalactic Lyα Nebulae at Cosmic Noon
Published 2024-01-01Get full text
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Bayesian Approach to Equipartition Estimation of Magnetic Field Strength
Published 2025-01-01Get full text
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