High-energy astrophysics
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- Shock breakout from mildly relativistic ejecta in a dense wind: the case of EP260321a/SN 2026gzf
- Quark and hybrid stars with renormalization group improvement of NNLO perturbative QCD
- Massive scalar fields in eccentric regime: Detectability and constraints from LISA observations of extreme mass-ratio inspirals
- Fermi-eROSITA cross-correlations suggest annihilation lines of ∼70 GeV WIMPs
- Transitions in the Mass-ratio and Spin Properties of Binary Black Holes in GWTC-5
- Continuous mass ablation of planets engulfed in stellar envelopes
- Simulating the jittering-jets explosion mechanism: circum-jet rings account for observed core-collapse supernova remnant morphologies
- Shortening the baseline: characterising Type Ia supernovae using Δ m 10( X )
- Probing Globular Clusters using Gravitational Waves from Inspiraling Stellar-mass Binary Black Holes in Space-based Detector
- A Search for High-energy Counterparts of Fast Radio Bursts
- Gamma-rays from black hole coronae: disentangling the leptonic and hadronic contributions
- A weakly modelled view of the joint compact-binary mass plane: population structure and spectral-siren cosmology
- Deep Learning for Cherenkov Astronomy: Performance of GammaLearn on LST-1
- An All-Sky Search for Moving Gamma-Ray Sources with Fermi-LAT
- Toward a complete understanding of the properties of GW190521
- A method for multimodal analysis of TAIGA experiment data using essential features
- Can LISA See Inside the Little Red Dots?
- Predictions for Short Gamma-Ray Burst Detections by COSI
- A Newly Identified Transient Ultraluminous X-ray Source in M31
- Modeling the nanohertz gravitational wave background with the t-process: Improved frequentist analysis of gravitational-wave power
- Extreme Stellar Death and Galaxy Feedback at z = 2: A Rest-frame Ultraviolet Characterization of the Strongly Lensed Superluminous Supernova 2025wny
- Unveiling the Accretion Architecture of GS 1354--64: A Broadband X-ray and Polarimetric Study of its 2025--2026 Outburst
- It Takes Two: nucleosynthesis in core-collapse supernova simulations of binary-star progenitors
- Constraining the gravitational-wave breathing mode with LVK antenna patterns and GWTC data
- Assessing transitional pulsar candidates through a quantitative estimation of their light-curve similarity