Journal of High Energy Astrophysics

Papers
(The H4-Index of Journal of High Energy Astrophysics is 20. The table below lists those papers that are above that threshold based on CrossRef citation counts [max. 250 papers]. The publications cover those that have been published in the past four years, i.e., from 2021-08-01 to 2025-08-01.)
ArticleCitations
An anthropic solution to the cosmological moduli problem754
GRB 080710: A narrow, structured jet showing a late, achromatic peak in the optical and infrared afterglow?135
Fermi-LAT and FAST observation of the gamma-ray binary HESS J0632+05768
Energetic requirements of the gamma-ray emission from pulsars: A nonparametric analysis of the data in the Fermi-LAT 12-Year Catalog65
Gamma-ray bursts calibrated from the observational H(z) data in artificial neural network framework53
Scalar's quasibound states in cosmological black hole background51
Constraints on anisotropic properties of the universe in f(Q,T) gravity theory48
Probing the warped vacuum geometry around a Kerr black hole by quasi-periodic oscillations38
An explanation of the muon puzzle of ultrahigh-energy cosmic rays and the role of the Forward Physics Facility for model improvement35
Dark energy and cosmic evolution: A study in f(R,T) gravity34
Interacting dark energy in curved FLRW spacetime from Weyl Integrable Spacetime32
Variability study of classical supergiant X-ray binary 4U 1907+09 using NuSTAR27
Studying the role of supernova remnants as cosmic ray PeVatron with LHAASO observations26
Evidence for extreme PeV cosmic ray acceleration from LHAASO25
Black holes immersed in polytropic scalar field gas24
Corrigendum to “LEIA in Flight Performance and Variability of Flux and Spectra of Some Bright X-ray Sources in the Galactic Plane” [Journal of High Energy Astrophysics,Volume 47, Article Number, 1003724
Observational constraints on extended Starobinsky and Weyl gravity model of inflation23
Observational analysis of late-time acceleration in f(Q,L) gravity22
Conservative wormholes in generalized κ(R21
Cooling of neutron stars in soft X-ray transients with realistic crust composition20
0.018608093261719