Cosmology
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- Unification of polynomial and exponential cosmological attractors
- Halo-driven Origin and Evolution of Overmassive Black Holes and Little Red Dots
- Exploring the dark sector through galaxy dynamics in clusters
- Initial conditions for inflation
- Macroscopic dark matter constraints for extended mass functions
- High-sensitivity Ultralight Dark Matter detector: Parametrically Amplified Casimir Devices
- Halo mass, star formation, and morphology in galaxies: A morphology-dependent connection between halo environment and star formation activity
- How Cluster Pressure Profiles Scale: Mass, Redshift, and Intrinsic Scatter
- Fast Lensing And Sub-minute High-accuracy photometry (FLASH) with JWST: Pipeline and Primordial Black Hole Microlensing Constraints from M31
- Analytic bispectrum covariance for galaxy survey cosmology
- Probing Dark Matter with Strongly Lensed Binary Black Hole Mergers: Prospects in the Near Future
- Expanding the scope of dark siren cosmology: Inferring the population properties of gravitational wave-hosting galaxies
- A guide to choosing data compression methods for cosmological inference
- Studies on the dark sector interaction from joint analysis of cosmological probes
- Revisiting the Hubble tension with an inverse power-law early dark energy
- Hubble tension: the shape wall
- UV artefacts in ultra-slow-roll models of inflation
- VROOM-SBI: A Fast Simulation-Based Bayesian Inference Methodology for Stokes QU-Fitting in Radio Interferometry
- Euclid. A two-point correlation approach to diagnosing star-related systematics in the Euclid spectroscopic survey
- Energy deposited by black holes in the hot X-ray gas of elliptical galaxies, groups and clusters
- Constraints on the inflationary vacuum and reheating era from NANOGrav
- Cosmological Constraints on Interacting Scalar-Field Dark Matter and Early Dark Energy mediated by a Kinetic Kernel
- Cosmological constraints on the interacting viscous dark matter and decaying vacuum energy models
- Inelastic Signatures of Electroweak Dark Matter
- H I Absorbers as Beacons of Hidden Structure at z ∼ 3: Multi-Component, Metal-Rich Absorption System near a Protocluster