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- A magnetically heated slim disc-corona model for tidal disruption events
- Chemical abundances of a Galactic Centre ejecta discovered in DESI
- A Massive and Eccentric Binary Millisecond Pulsar in the Globular Cluster M10
- Jovian Polar Vortex Generation in a Shallow-Water Model with Quasi-Stochastic Convection
- A Century-Long Archival Search and Analysis of the Rubin Observatory-Discovered Dwarf Planet Candidate 2026 ED138
- Imaging the Current Distribution in Superconducting Transition-Edge Sensors with Scanning SQUID Microscopy
- Harmonic Angular Mapping Method for Binary Microlensing Grid Search
- The Transient Array Radio Telescope: An open-source all-sky imaging radio interferometer
- The imprint of individual neutron star spins on ejecta, r-process nucleosynthesis, and kilonovae in binary neutron star mergers
- Sub-sonic compressible magnetohydrodynamic turbulence I. Alfvénic and fast-magnetosonic injection, amplitude dependence, and compressibility effects
- Extending dynamical mass measurements: probing GI as a possible origin of mm-dust spirals
- High resolution Lyman-α forest constraints on dark matter-neutrino scattering
- Cosmogenic photon fluxes at ultra-high energies
- Ultra-High-Energy Cosmic Ray Boosted Relic Neutrinos
- First Light and Reionization Epoch Simulations (FLARES) XXII: UV-dust spatial offsets at the Epoch of Reionisation
- A New Global Chemical Equilibrium Code: Refractory Element Signatures in Super-Earths and Sub-Neptunes
- The Quantum Noise Fraction and the addressable fraction in High-Frequency Gravitational Wave Detection
- Reduced Gravitational Wave Signal Reopens the Ultralight Primordial Black Hole Window
- Multiepoch Stability in the Rotational Modulation of the Planetary-mass Companion Ross 458C
- Quantifying the Dominance and Emergence of Brightest Cluster Galaxies in SPT and Planck Clusters: A Novel Application of the Gini Index
- First Measurement of the Hubble Constant from Gravitational Wave–Galaxy Cross Correlations
- Inside the cocoon: A comprehensive explanation of the spectra of little red dots
- GLOW. I. Comprehensive Measurements of Gas-rich, Star-forming, Low-mass Galaxies in the Nearby Universe*
- Where Galaxies Go to Die: The Environments of Massive Quiescent Galaxies at 3 < z < 5
- Accretion Rates and Thermohaline Convection in Polluted White Dwarfs