Gaussian process reconstruction of scalar field dynamics from recent cosmological data
astro-ph.CO
Submitted: 2026-08-25
Updated: 2026-08-25
Terminology
Sources
- Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
- Measurements of Omega and Lambda from 42 High-Redshift Supernovae
- The Complete Light-curve Sample of Spectroscopically Confirmed Type Ia Supernovae from Pan-STARRS1 and Cosmological Constraints from The Combined Pantheon Sample
- The Pantheon+ Analysis: Cosmological Constraints
- Union Through UNITY: Cosmology with 2,000 SNe Using a Unified Bayesian Framework
- The Dark Energy Survey: Cosmology Results With ~1500 New High-redshift Type Ia Supernovae Using The Full 5-year Dataset
- Planck 2013 results. XVI. Cosmological parameters
- Planck 2018 results. VI. Cosmological parameters
- DESI 2024: Constraints on Physics-Focused Aspects of Dark Energy using DESI DR1 BAO Data
- DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints
- The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: measurement of the growth rate of structure from the anisotropic correlation function between redshift 0.8 and 2.2
- The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample
- Baryon acoustic oscillations from the complete SDSS-III Ly$\alpha$-quasar cross-correlation function at $z=2.4$
- DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations
- DESI 2024 III: Baryon Acoustic Oscillations from Galaxies and Quasars
- DESI 2024 IV: Baryon Acoustic Oscillations from the Lyman Alpha Forest
- DESI 2024: Reconstructing Dark Energy using Crossing Statistics with DESI DR1 BAO data
- Cosmic Chronometers: Constraining the Equation of State of Dark Energy. I: H(z) Measurements
- Improved constraints on the expansion rate of the Universe up to z~1.1 from the spectroscopic evolution of cosmic chronometers
- Setting the Stage for Cosmic Chronometers. II. Impact of Stellar Population Synthesis Models Systematics and Full Covariance Matrix
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