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- Temporal rhythms of uncertainty: Evaluating Mars claims in the Australian colonial press
- Post-fragmentation Morphological and Broadband Color Evolution of C/2025 K1 (ATLAS)
- A MAGNHIFFIC cold-gas filament fuelling the nuclear activity of NGC 3100
- AllBRICQS: the All-sky BRIght, Complete Quasar Survey - Quasar Selection and Final Southern GRP<16 Sample
- Polar-structure galaxies beyond the local Universe: first results from Euclid
- Halo formation and distribution around cosmic web
- Atmospheric Turbulence Profiling in the Lenghu Site Area Using MERRA-2 Data
- Comment on "Effect of perfect fluid dark matter..." [Phys. Dark Univ. 34 (2021) 100891]
- Observational evidence of the Gaia-Enceladus-Sausage merger's influence on the opposite side of the Galactic Center
- Properties of Oxygen-rich Asymptotic Giant Branch stars in the LMC and the Milky Way
- MACE: Multigroup-Multiangle Integrated Thermal Compton Scattering Kernel
- Clustering of JWST LRDs. Implications for PBHs and other early-forming seeds
- The Redshift-Space Galaxy Power Spectrum at Two-Loop Order
- The Neutral Hydrogen Gas Content of Star-forming and Quiescent S0 Galaxies
- Black Hole Spacetime Reconstruction from Galactic Rotation Curves: Thermodynamic Properties and Implications
- Breakout/Interchange Reconnection as a driver of Jets, Fast Coronal Mass Ejection, and Solar Energetic Particles
- Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics
- No evidence for a supermassive black hole binary in GSN 069
- Asteroseismic forward modelling of 36 β Cep pulsators and inferences on their internal differential rotation
- Sublimation-driven fragmentation of icy dust aggregates in main-belt comets
- The properties of central stellar knots embedded in galactic bulges of CIELO simulations
- Candidates for the most [O III]λ5007-luminous planetary nebula in the Milky Way
- Self-gravity in thin protoplanetary discs
- New galaxy cluster in the zone of avoidance SRGe CL0512.7+3712
- Vera C. Rubin LSST synthetic magnitudes derived from Gaia XP spectra