Universe Expansion Big Crunch DESI Supernovae Black Holes Cosmic Expansion Research Findings Expansion Rate Dark Energy Spectroscopic Instrument Hubble Tension Type Ia Supernovae Universe Mapping Cosmological Constant DESI Collaboration Nature of Dark Energy Dark Matter Dynamical Dark Energy Dark Energy Camera Data Analysis Implications Future of the Universe Dark Energy Survey Dark Energy Theories Euclid Space Telescope Dark Energy Spectroscopy Instrument Dark Energy Effect Evolution Effects on Universe Expansion Artificial Intelligence Simulations Dark Energy Discovery Evolution over Time Desi Baryonic Matter Acoustic Oscillations Lambda CDM Model Quasars DESI Instrument Evolving Nature Supernova Brightness Galaxies DESI Project Properties Expansion of the Universe Standard Candles Evolving Dark Energy Cosmic Mysteries Universe Exploration Universe Lifespan Cosmic Phenomena Dynamical Dark Energy Models Axions Dynamical Models Dark Energy Dynamics Peculiar Velocities Cosmological Models Euclid Observations Evolution of Dark Energy Interacting Dark Energy Models Baryon Acoustic Oscillations Galaxy Catalogs $ ext{w}_0 ext{w}_a ext{CDM}$ Cosmic Evolution Type Ia Supernovas Gaussian Process Regression Large-Scale Structure Cosmic Voids Lensing Measurements Galaxy Clustering Universal Expansion Big Rip Theory Big Crunch Theory Exoplanets Observational Techniques Theories and Mysteries Holographic Dark Matter Gravitational Lensing Star Formation Drake Equation Intelligent Life Expansion History of the Universe General Relativity Dark Universe Universe Dynamics Timescape Model Cosmic History International Research Efforts Galactic Studies Observational Studies Dark Energy Evolution Observational Cosmology Cosmic Fate Cosmological Theories
The fully assembled observatory is in final testing ahead of a planned 2027 launch.
