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- Interaction of Stellar Dipole and Disk Magnetic Fields in Accretion–Ejection Systems
- From Cluster Cores to the Low-density Field: Strong Environmental Quenching of Galaxy Star Formation at Low Redshift
- Early Near-IR Echo and the Time-variable Mass-loss History of Type IIn SN 2024kgi
- Phase-dependent Magnetic Coherence in the Turbulent Interstellar Medium
- Hierarchical Hub Formation in Mon R2: Evidence for Cloud-to-core Gas Flows
- Convolutional Neural Network for Extraction of n = 1 Photon Ring of Black Holes
- The Role of Nonlocal Thermal Transport in Flare-driven Chromospheric Evaporation
- Eclipse Properties and Superhump Evolution in the SU UMa-type Dwarf Nova Z Cha
- Black Hole Supernovae Outcomes Across a Wide Progenitor Range
- Hard X-Ray Quasiperiodic Pulsations in X-class Solar Flares Observed by Aditya-L1/HEL1OS
- Mid-infrared Diagnostics of Polycyclic Aromatic Hydrocarbon Processing and Radiation Fields in M33 H II Regions with JWST/MIRI
- What Drives Galaxy–Galaxy Differences in the Selective Attenuation Curve? New Perspectives from DESI DR1
- The KAGG Survey: KCWI Analysis of Gas around Galaxies at z ≈ 3–5
- Dust Growth in Evolving Filamentary Molecular Clouds: Signatures in Ionization, Resistivity, and Infrared Scattering
- GraphShed: A Data-derived Graph-based Watershed Group-finder
- Evolution of the High-energy Excess in Swift J1727.8-1613 during Its 2023 Flare State
- First Statistical Analysis of Photospheric Intensity Vortices with DKIST/VBI
- Probing the All-sky Distribution of Soft X-Ray Emission Associated with the Milky Way
- A Massive Barred Spiral Galaxy at z = 5.102 Discovered by JWST
- Delayed Feedback in High-z Starbursts Revealed by Lyα Profiles and Metal-line Diagnostics
- Electron Acceleration by Turbulent Reconnection in Solar Flares
- Thermal Stability of Radiation-pressure-dominated Accretion Disks Threaded by Net Vertical Magnetic Flux
- Lightweight CNN and transformer detectors for real-time single-fruit date-variety recognition on edge GPU hardware
- Present-day coasting in a flat FLRW cosmology with a transient acceleration pocket
- Fine and ultrafine Martian dust presents additional risks for future crewed missions to Mars