Cosmology
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- An obstruction to cosmic acceleration from shift-symmetric dark sector interactions
- DESI DR2 Results III: The Mass of the Milky Way
- Gravitational waves flooding the Universe after wall domination
- Euclid: Forecasting the number counts of bright line emitters in the Euclid Wide Survey and Euclid Deep fields
- Euclid. Predicting scaling relations for emission-line galaxies using simulated data
- CHEX-MATE: Density profile reconstruction in galaxy clusters
- Dynamics of self-gravitating halos with decaying dark matter
- The Start Time of Ringdown
- CosmoVerse Data Challenge: How Tip of the Red Giant Branch Analysis Choices Shape the Inferred Hubble Constant
- The PAU Survey: Self-supervised image denoising for flux-preserving photometry
- Gravitational Wave Birefringence in generalized Palatini Chern Simons
- SBi3PCF: cosmology with Dark Energy Survey Year 3 cosmic shear
- Mapping large-scale structure without galaxy formation - combining fast radio bursts with CMB lensing
- Bright Siren Cosmology Beyond Fisher: DALI Forecasts for Third-Generation Gravitational Wave Observatories
- Response to "Late Time Dynamical Dark Energy and the CMB-Distance Ladder Tension"
- Cosmological evolution and late-time attractors in axion-monopole interacting dark energy
- Macrocanonical Generator Networks: Data-Efficient Neural Surrogates for Amortized Physics Simulation
- Gravitational-wave lensing beyond the diffraction integral: proper-time methods and the bound lens
- Linear perturbation theory and structure formation in a Horndeski theory of gravity without dark matter
- Reconstructing the Large-Scale Velocity Field from DESI DR1 with Bayesian Inference
- Structural axes of sources in the SUMSS survey and their alignments
- Stress-Testing Small-Scale Cosmological Inference With Empirical Galaxy--Halo Connection Models
- Measuring the ultraviolet background at z≃3 from the quasar proximity effect in DESI DR1
- Comment on "Long-range magnetic fields in the ground state of the Standard Model plasma"
- Sample Variance Cancellation for Future Spectroscopic Surveys