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- A New Framework for Modeling Solar Flares from Magnetohydrodynamic to Kinetic Processes
- Eight Gamma-Ray Bursts Observed with the Fermi Gamma-Ray Burst Monitor: Significant Quasi-thermal Components and Conditional Jet Constraints
- Impact of Upstream Clumpiness on Supernova Remnant Forward Shock Evolution in Molecular Cloud Environments
- Joint Multiband Photometry with crowdsource
- An Exploration of In-band Spectral Index Techniques for Extended Radio Sources with EMU
- Coevolution of Dust Growth and Gravitational Instability in Massive Protostellar Disks
- Stellar Collisions from Self-consistent Stellar Dynamics around Growing Supermassive Black Holes
- Planetary Accretion Is Less Frequent in Wide Binaries: Evidence from Metal-enriched White Dwarfs in DESI DR1
- Damping and Dispersion of Acoustic Waves in the Solar Corona
- Quantifying and testing the evidence for a phantom crossing
- Two-Fluid Radial Stability of Dark-Matter-Admixed Compact Objects: Dark Compact Planets, Dark White Dwarfs, Dark Neutron Stars, and Dark Oysters
- Vacuum Phase Transition and Decay to Cross the Phantom Divide
- An Assessment of Water Vapor Radiometry Landscape in ngVLA Context
- Machine Learning Sensor Fusion for Water Vapor Radiometry based Tropospheric Delay Calibration
- GRB 241113B: the first SVOM and EP gamma-ray burst A soft GRB likely seen on-axis, from soft X-rays to gamma-rays
- Completeness and dynamical stability in exoplanet occurrence rates
- Optimizing Prompt Radio Counterpart Searches for Gravitational-Wave Events with the Deep Synoptic Array
- The Size-Mass Relation and Inside-Out Quenching of Massive Quiescent Galaxies at 2<z<3 with JWST PRIMER and MINERVA
- Equipartition between Alfvénic turbulence and energetic ions as the origin of the -5 common spectrum in the heliosphere
- The Importance of Curium-250 to the γ-Ray Signature of r-Process Remnants
- Stars Can Quench Superradiance Around Supermassive Black Holes
- Stress-enhanced diffusion in Yukawa crystals
- FOMO-Z. Optimal galaxy classification, photometric redshifts, and reconstruction of population distributions
- From Quantum Field Fluctuations to High-Redshift AGN: Semiclassical Origins of Halo Mass Function Constraints in the JWST Era
- NGDEEP: Anchoring the 0.5 < z < 3.5 Star-Forming Main Sequence at Low Stellar Masses with Ultradeep JWST/NIRISS WFSS