Universe Expansion Big Crunch Dark Energy Survey Cosmic Expansion Black Holes Dark Energy Spectroscopic Instrument Supernovae DESI Research Findings Expansion Rate Dark Energy Camera Type Ia Supernovae Dynamical Dark Energy Cosmological Models Galaxies Galaxy Clustering Nature of Dark Energy Dark Matter DESI Collaboration Implications Future of the Universe Dark Energy Spectroscopy Instrument Hubble Tension Data Analysis Cosmological Constant Cosmological Theories Universe Mapping Dark Energy Theories Standard Candles Baryon Acoustic Oscillations Cosmic Evolution Lambda-CDM Model Theoretical Physics Cosmic History Accelerating Universe Dark Energy Effect Universe Lifespan Drake Equation Einstein-Euler Equations Evolution of Dark Energy New Physics Cosmic Fate Acoustic Oscillations Expansion History of the Universe Peculiar Velocities Lambda CDM Model Dark Energy Evolution DESI Project Dynamical Models DESI Instrument Implications for Cosmology Evolution over Time $ ext{w}_0 ext{w}_a ext{CDM}$ Star Formation Cosmic Distance-Redshift Relation Dynamical Dark Energy Models Supernovae as Distance Indicators Big Crunch Theory Cosmic Mysteries Cosmic Phenomena HETDEX Project Observational Studies Intelligent Life Type Ia Supernovas Observational Techniques Cosmic Voids Gravitational Lensing Timescape Model Observational Cosmology Cosmological Measurements Exoplanets Theories and Mysteries Dark Energy Dynamics Artificial Intelligence Euclid Observations Universal Expansion Cosmologically Coupled Black Holes Dark Universe Universe Exploration Holographic Dark Matter Interacting Dark Energy Models Dark Energy Discovery Axions Supernova Brightness Baryonic Matter Evolution Universe Dynamics Galaxy Catalogs Weak Lensing Desi Euclid Space Telescope General Relativity Simulations Properties 3D Mapping of the Universe Evolving Nature International Research Efforts Observational Methods Big Rip Theory Effects on Universe Expansion
The papers conflict because they apply different corrections to the same Pantheon+ supernova sample and say much larger Rubin/LSST data will be needed to decide which method is right.
