Cosmology
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- A new H0 measurement with SNe Requiem and Encore using Gravity.jl
- Singlet-doublet dark matter induced radiative neutrino mass and TeV scale leptogenesis
- COSMOS-3D: Diverse Environments and Hot-dust Signatures among Dusty Star-forming Galaxies at z = 4.9-7.2
- ViCTORIA project: A pilot study of the M49 region in the Virgo cluster in polarisation
- The separate universe approach with non minimal coupling to gravity
- Probing Baryons with the Kinematic Sunyae Zel'dovich Effect and Machine Learning Derived Peculiar Velocities using DESI DR2 and ACT DR6
- Field-level inference of growth rate from DESI BGS galaxy and ZTF supernova simulations
- Lidar-monitoring of atmospheric fluctuations for millimeter-wave astronomical observations
- Constraining the galaxy-halo connection at z>10 using the neighbors of UV-bright galaxies
- Observations of Repeating Tidal Disruption Events
- Dark energy and negative compressibility of the Universe: A study based on cosmic equations of state
- JWST evidence for a sharp "Cosmic Daybreak" at z = 15
- Do primordial quark pellets solve the dark matter puzzle?
- Constant-Roll Inflation as a Competitive Alternative to Slow-Roll Inflation
- Cool Embeddings: Predicting Galaxy Cluster Cooling Times in IllustrisTNG and TNG-Cluster with AstroCLIP
- Bimodal mass primordial black holes in three-field inflation
- Exact Solutions for Chiral Gravitational Waves from Spin-2 Mixing
- AGN hosting jets. II: Deriving fundamental information from semi-analytical models and the LoTSS sample
- Observing population III stars in the pristine region
- The Physical Origins of Scatter in the Dust Attenuation Scaling Relation of Star-Forming Galaxies: Star--Dust Geometry
- Universality classes of sharp gravitational production of light particles
- Cross-correlation between CMB B-modes and Faraday Rotation as a Novel Probe of Primordial Magnetic Fields
- Falsifiable anthropic model from the string landscape
- Turbulent Transport of Galactic Magnetic Fields into Cosmic Voids: Insights from IllustrisTNG
- Galaxy and Halo Assembly Bias in Alternative Dark Matter Models