Perspective of monochromatic gamma-ray line detection with the High Energy...
HERD is the High Energy cosmic-Radiation Detection instrument proposed to operate onboard China's space station in the 2020s. It is designed to detect energetic cosmic ray nuclei, leptons and photons...
View ArticleAccelerator measurements of magnetically-induced radio emission from particle...
For fifty years, cosmic-ray air showers have been detected by their radio emission. We present the first laboratory measurements that validate electrodynamics simulations used in air shower modeling....
View ArticleApplication of Bayesian Neural Networks to Energy Reconstruction in EAS...
A toy detector array has been designed to simulate the detection of cosmic rays in Extended Air Shower(EAS) Experiments for ground-based TeV Astrophysics. The primary energies of protons from the...
View ArticleIntegration of Particle-Gas Systems with Stiff Mutual Drag Interaction...
Numerical simulation of numerous mm/cm-sized particles embedded in a gaseous disk has become an important tool in the study of planet formation and in understanding the dust distribution in observed...
View ArticleMission to the Gravitational Focus of the Sun: A Critical Analysis [Replacement]
The gravitational field of the sun will focus light from a distant source to a focal point at a minimal distance of 550 Astronomical Units from the sun. A proposed mission to this gravitational focus...
View ArticleStatistical properties of Fourier-based time-lag estimates [Replacement]
The study of X-ray time-lag spectra in active galactic nuclei (AGN) is currently an active research area, since it has the potential to illuminate the physics and geometry of the innermost region (i.e....
View ArticleNIKEL_AMC: Readout electronics for the NIKA2 experiment [Replacement]
The New Iram Kid Arrays-2 (NIKA2) instrument, dedicated to mm-wave astronomy, uses microwave kinetic inductance detectors (KID) as sensors. The three arrays installed in the camera feature a total of...
View ArticleImplementation and performance of FDPS: A Framework Developing Parallel...
We present the basic idea, implementation, measured performance and performance model of FDPS (Framework for developing particle simulators). FDPS is an application-development framework which helps...
View ArticleSolar neutrino detection in a large volume double-phase liquid argon...
Precision measurements of solar neutrinos emitted by specific nuclear reaction chains in the Sun are of great interest for developing an improved understanding of star formation and evolution. Given...
View ArticleA Causal, Data-Driven Approach to Modeling the Kepler Data [Replacement]
Astronomical observations are affected by several kinds of noise, each with its own causal source; there is photon noise, stochastic source variability, and residuals coming from imperfect calibration...
View ArticleThe DES Science Verification Weak Lensing Shear Catalogues [Replacement]
We present weak lensing shear catalogues for 139 square degrees of data taken during the Science Verification (SV) time for the new Dark Energy Camera (DECam) being used for the Dark Energy Survey...
View ArticleThe Point Spread Function Reconstruction by Using Moffatlets – I
The shear measurement is a crucial task in the current and the future weak lensing survey projects. And the reconstruction of the point spread function(PSF) is one of the essential steps. In this work,...
View ArticleMOCCA code for star cluster simulations – VI. Bimodal spatial distribution of...
The paper presents an analysis of formation mechanism and properties of spatial distributions of blue stragglers in evolving globular clusters, based on numerical simulations done with the MOCCA code....
View ArticleMission to the Gravitational Focus of the Sun: A Critical Analysis [Replacement]
The gravitational field of the sun will focus light from a distant source to a focal point at a minimal distance of 550 Astronomical Units from the sun. A proposed mission to this gravitational focus...
View ArticleMOCCA code for star cluster simulations – V. Initial globular cluster...
The paper presents an analysis of properties of populations of blue stragglers (BSs) in evolving globular clusters, based on numerical simulations done with the MOCCA code for various initial globular...
View ArticleBeyond the diffraction limit via optical amplification
In a previous article we suggested a method to overcome the diffraction limit behind a telescope. We refer to theory and recent numerical simulations, and test whether it is indeed possible to use...
View ArticleSolar neutrino detection in a large volume double-phase liquid argon...
Precision measurements of solar neutrinos emitted by specific nuclear reaction chains in the Sun are of great interest for developing an improved understanding of star formation and evolution. Given...
View ArticleAssessment of backgrounds of the ANAIS experiment for dark matter direct...
A large effort has been carried out to characterize the background of sodium iodide crystals within the ANAIS (Annual modulation with NaI Scintillators) project. In this paper, the background models...
View ArticleAccurate abundance analysis of late-type stars: advances in atomic physics
The measurement of stellar properties such as chemical compositions, masses and ages, through stellar spectra, is a fundamental problem in astrophysics. Progress in the understanding, calculation and...
View ArticleA Close Examination of the Measurement and Parametrization of Luminosity...
The astronomy community has at its disposal a large back catalog of public spectroscopic galaxy redshift surveys that can be used for the measurement of luminosity functions. Utilizing the back catalog...
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