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- Effects of Eddington-inspired Born-Infeld Gravity on Black Hole Accretion
- Kinematic Decomposition of the BCG and ICL in Abell S1063 and MACS J1206
- The assembly of dusty galaxies at z ≥ 4: grain growth and the evolutionary origin of the dust-to-stellar-mass scatter
- Learning Galaxy Kinematics from Spatially Unresolved Spectra
- How to feed your dragon: the role of turbulence in AGN activity
- Cosmic merger rates and population evolution of binary black hole mergers in AGN disks
- Model-independent and reconstruction-free evidence for cosmic acceleration from DESI baryon acoustic oscillations
- Bridging Scales: Multi-Zone GRMHD-Informed Anisotropic AGN Feedback in Galaxies
- Missing Mergers: On the Unexpected Delay-Time Distribution of Binary Neutron Star Mergers
- Leaking Sound Waves: Gravitational Waves From Dark Sectors Weakly Coupled to the Standard Model
- On the Role of Gravity in Supercooled Phase Transitions
- Surprisingly normal? GW241011 and GW241110 in the context of hierarchical merger classification
- When precise inference is wrong: Diagnosing model misspecification with applications to cosmic dawn and reionisation
- Chaos and loss: reevaluating the loss-cone formalism in the context of chaotic diving orbits in flattened potentials
- Hints of self-interacting dark matter from strong gravitational lensing
- SEAMLESS Survey: A Closer Look at Seven Local Volume Dwarf Galaxies in Diverse Environments
- Likely Metal Scarring in the Magnetic White Dwarf LHS 2534
- Optimizing the extraction of information from redshift probability distribution functions
- Supergranulation as a Tracer of Solar-Cycle Variability
- Corrected detector-level reconstruction of inclined radio air showers from trigger-level ADC waveforms
- What becomes of JWST/NIRCam-selected high-redshift massive galaxies?
- The Status of Single Scalar Field Dark Energy
- Curvature-Radiation Geometries Across the Second CHIME/FRB Fast Radio Burst Population
- Stability of circumbinary planets: The role of binary properties and migration scenarios
- The δ Scuti instability strip and period-luminosity relation as seen by TESS and Gaia DR3