Cosmology
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- Mass Proxy Quality of Halo Properties in IllustrisTNG and FLAMINGO Simulations: II. Galaxies, Stars, and Black Holes
- An LSST-DESC Precursor Project: Hyper Suprime-Cam Year 1 3×2pt in Harmonic Space
- Joint Model-independent Constraints on the Post-Newtonian Parameter and Cosmic Curvature from Galaxy-scale Strong Lensing, SNe Ia, BAO, and Cosmic Chronometers
- Gravitational wave echoes as probes of the maximum mass of strange stars in quadratic curvature-matter coupled gravity
- Particle production from bubble collisions
- Fire at the Tip of the Throat: Hagedorn Phase after brane-antibrane inflation?
- Real versus Complex Fermion Bare Mass and Multi-Wall String Defect Annihilation
- Observing the Peculiar Acceleration of our Solar System with Quasar Proper Motions
- Exploring non-Poisson satellite occupation in HOD models and its impact on 2- and 3-point galaxy clustering
- Inpainting to search for premerger massive black hole binaries in realistic LISA datasets
- Parameterizations of the Hubble Constant from the Binned Type Ia Supernova Master Sample: Logarithmic versus Power-law Forms
- Cosmological constraining power of the redshifts, heights, and angular clustering of weak gravitational lensing peaks
- Stochastic gravitational waves from narrow-band cosmological magnetic fields
- The road to H0, Ωm, and w with a global neutrino-telescope network
- Seeing in the Dark: Gravitational Waves from Resonant Production of Dark Photon Dark Matter
- A Burst of Reionization in the Dark Ages
- Galaxy Clustering Can Reveal Host-Galaxy Properties of Binary Black Hole Mergers
- Reconstructing Early Primordial Black Hole Domination from Gravitational-Wave Backgrounds
- Statistical Field Theory for Weak Gravitational Lensing
- A Pairwise Surrogate for Gravitational-Wave Spectra from Highly Relativistic Vacuum Bubble Collisions
- Opening the Black Box: What Neural Networks Learn from Pulsar Timing Array Data
- An analytical model for non-local stochastic field-level galaxy bias on the sphere
- Modeling CO Line Luminosity Using FIRE Simulations: I. Methodology and Validation of Molecular Gas and CO Abundance
- Too many or too bright? Status and perspectives in the study of the UV Luminosity Function at z>10
- A New Era for Supernova Science with the James Webb Space Telescope