Euclid. I. Overview of the Euclid mission

Abstract

The current standard model of cosmology successfully describes a variety of measurements, but the nature of its main ingredients, dark matter and dark energy, remains unknown. Euclid is a medium-class mission in the Cosmic Vision 2015-2025 programme of the European Space Agency (ESA) that will provide high-resolution optical imaging, as well as near-infrared imaging and spectroscopy, over about 14,000 deg^2 of extragalactic sky. In addition to accurate weak lensing and clustering measurements that probe structure formation over half of the age of the Universe, its primary probes for cosmology, these exquisite data will enable a wide range of science. This paper provides a high-level overview of the mission, summarising the survey characteristics, the various data-processing steps, and data products. We also highlight the main science objectives and expected performance.

Accepted for publication in the A&A special issue`Euclid on Sky'

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• Extending the supernova Hubble diagram to z~1.5 with the Euclid space mission
• The WiggleZ Dark Energy Survey: Final Data Release and the Metallicity of UV-Luminous Galaxies
• A direct measurement of galaxy major and minor merger rates and stellar mass accretion histories at $z<3$ using galaxy pairs in the REFINE survey
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• Probing large scale coherence between Spitzer IR and Chandra X-ray source-subtracted cosmic backgrounds
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• A combined VANDELS and LEGA-C study: the evolution of quiescent galaxy size, stellar mass and age from $\text{z}=0.6$ to $\text{z}=1.3$
• First results from GeMS/GSAOI for project SUNBIRD: Supernovae UNmasked By Infra-Red Detection
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• Euclid preparation: XLVIII. The pre-launch Science Ground Segment simulation framework
• Euclid preparation. XXVII. A UV-NIR spectral atlas of compact planetary nebulae for wavelength calibration
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• Exponential quintessence with momentum coupling to dark matter
• Euclid: The potential of slitless infrared spectroscopy: A z=5.4 quasar and new ultracool dwarfs
• Free-floating planetary mass objects in LDN 1495 from Euclid Early Release Observations
• Euclid preparation. Simulating thousands of Euclid spectroscopic skies
• AMICO galaxy clusters in KiDS-1000: cosmological constraints and mass calibration from counts and weak lensing
• Updated Cosmological Constraints from 2D BAO Measurements: A New Compilation and Comparison with DESI DR2
• Euclid preparation. Spatially resolved stellar populations of local galaxies with Euclid: a proof of concept using synthetic images with the TNG50 simulation
• Shedding light on the star formation rate-halo accretion rate connection and halo quenching mechanism via DECODE, the Discrete statistical sEmi-empiriCal mODEl
• The COSMOS-Web Lens Survey (COWLS) III: forecasts versus data
• HOLISMOKES XV. Search for strong gravitational lenses combining ground-based and space-based imaging
• The SRG/eROSITA All-Sky Survey. The Weak-Lensing Mass Calibration and the Stellar Mass-to-Halo Mass Relation from the Hyper Suprime-Cam Subaru Strategic Program
• Euclid: Early Release Observations of ram-pressure stripping in the Perseus cluster. Detection of parsec scale star formation with in the low surface brightness stripped tails of UGC 2665 and MCG +07-07-070
• Millimeter-wave observations of Euclid Deep Field South using the South Pole Telescope: A data release of temperature maps and catalogs
• The Ly$\alpha$ and Continuum Origins Survey. III. Investigating the Link between Galaxy Morphology, Merger Properties and LyC Escape
• The VMC survey -- LIII. Data release #7. Complete survey data and data from additional programmes
• $H_0$ Without the Sound Horizon (or Supernovae): A 2% Measurement in DESI DR1
• Measuring our peculiar velocity from spectroscopic redshift surveys
• pop-cosmos: Insights from generative modeling of a deep, infrared-selected galaxy population
• Modeling spatially-resolved galactic H$\alpha$ emission for galaxy clustering
• Euclid: Photometric redshift calibration with self-organising maps
• When Dark Matter Heats Up: A Model-Independent Search for Non-Cold Behavior
• Learning the Universe: Learning to Optimize Cosmic Initial Conditions with Non-Differentiable Structure Formation Models
• Euclid preparation. The impact of relativistic redshift-space distortions on two-point clustering statistics from the Euclid wide spectroscopic survey
• Euclid preparation. Exploring the properties of proto-clusters in the Simulated Euclid Wide Survey
• Searching for strong lensing by late-type galaxies in UNIONS
• KiDS-1000: Detection of deviations from a purely cold dark matter power spectrum with tomographic weak gravitational lensing
• From Large Telescopes to the MUltiplexed Survey Telescope (MUST)
• The Host Galaxies of PTA Sources: Converting Supermassive BH Binary Parameters into EM Observables
• A frequentist view on the two-body decaying dark matter model
• Improving CMB constraints on early Universe physics with LSS: A multi-probe forecast including cross-covariance
• Principal Components for Model-Agnostic Modified Gravity with 3x2pt
• Extending evolution mapping to massive neutrinos with COMET
• Constraining galaxy properties with complete samples of lenses
• Euclid preparation. LXVII. Deep learning true galaxy morphologies for weak lensing shear bias calibration
• The case for an Astrometric Mission Extension of Euclid. Extending Gaia by 6 magnitudes with Euclid covering one-third of the sky
• The revolution in strong lensing discoveries from Euclid
• Revisiting the X-ray-to-UV relation of Quasars in the era of all-sky surveys
• DESI forecast for Dark Matter-Neutrino interactions using EFTofLSS
• Weak lensing constraints on the stellar-to-halo mass relation of galaxy groups with simulation-informed scatter
• A short review on Quintom dark energy theory
• LATIS: Comparing Galaxy and IGM Tomography Maps as Tracers of Large-scale Structure and Protoclusters at $z\sim 2.5$
• GalaxyGenius: Mock galaxy image generator for various telescopes from hydrodynamical simulations
• The Cosmological analysis of X-ray cluster surveys VII. Bypassing scaling relations with Lagrangian Deep Learning and Simulation-based inference
• The Effective Field Theory of Large Scale Structure for Mixed Dark Matter Scenarios
• Weak Gravitational Lensing
• Euclid preparation. 3-dimensional galaxy clustering in configuration space. Part I. 2-point correlation function estimation
• Separating Angular and Radial Modes with Spherical-Fourier Bessel Power Spectrum on All Scales and Implications for Systematics Mitigation
• Reconstructing galaxy star formation histories from COSMOS2020 photometry using simulation-based inference
• Galaxies OBserved as Low-luminosity Identified Nebulae (GOBLIN): a catalog of 43,000 high-probability dwarf galaxy candidates in the UNIONS survey
• Towards a Composite Framework for Simultaneous Exploration of New Physics in Background and Perturbed Universe
• 6x2pt: Forecasting gains from joint weak lensing and galaxy clustering analyses with spectroscopic-photometric galaxy cross-correlations
• Galactic bars and active galactic nucleus fuelling in the second half of cosmic history
• A Light-Cone Approach to Higher-Order Cosmological Observables
• Accreted stars and stellar haloes of simulated galaxies in TNG50
• Estimating infall times of galaxies around clusters: how accurately can it be done with observational data?
• The imprints of massive neutrinos on the three-point correlation function of large-scale structures
• Euclid: Constraints on f(R) cosmologies from the spectroscopic and photometric primary probes
• COUGS-DESI: A Catalog of Unusual Galaxies with Polar Structures in the DESI Legacy Imaging Surveys
• The AIDA-TNG project: 3D halo shapes
• The AIDA-TNG project: dark matter profiles and concentrations in alternative dark matter models
• On the tomographic cluster clustering as a cosmological probe
• Modelling the photometric and morphological evolution of disc galaxies in the cluster environment
• A Redshift Survey of the Coma Cluster (A1656): Understanding the Nature of Subhalos in the Weak-lensing Map
• Impact of weak-lensing mass-mapping algorithms on cosmology inference
• ULTIMATE-deblending I. A 50-band Ultraviolet to Mid-infrared Photometric Catalog Combining Space- and Ground-based Data in the JWST/PRIMER survey
• Dust-obscured Galaxies with Broken Power-law Spectral Energy Distributions Discovered by UNIONS
• Characterizing the outer disk of eXtended-UV galaxies in the optical domain with deep surveys
• Euclid Quick Data Release (Q1): The evolution of the passive-density and morphology-density relations between $z=0.25$ and $z=1$
• Impact of redshift distribution uncertainties on Lyman-break galaxy cosmological parameter inference
• Reconstructing redshift distributions with photometric galaxy clustering
• Euclid preparation. Estimating galaxy physical properties using CatBoost chained regressors with attention
• Euclid preparation: TBD. Cosmic Dawn Survey: evolution of the galaxy stellar mass function across 0.2<z<6.5 measured over 10 square degrees
• Redshift-space galaxy bispectrum in presence of massive neutrinos: A multipole expansion approach for Euclid
• Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics
• Analytical $poly\Lambda$CDM dynamics
• Echoes from the dark: Galaxy catalog incompleteness in standard siren cosmology
• Euclid: Early Release Observations -- The star cluster systems of the Local Group dwarf galaxies IC 10 and NGC 6822
• Star-forming galaxies in the cosmic web in the last 11 Gyr
• From Dark Radiation to Dark Energy: Unified Cosmological Evolution in K-essence Models
• Euclid preparation. Overview of Euclid infrared detector performance from ground tests
• On the Robustness of Cluster Clustering Covariance Calibration
• Blending effects on shear measurement synergy between Euclid-like and LSST-like surveys
• Pixelization effects in cosmic shear angular power spectra
• DUCA: Dynamic Universe Cosmological Analysis. I. The halo mass function in dynamical dark energy cosmologies
• Dusty Clump Survival in Supernova Ejecta: Dust-Mediated Growth vs. Crushing by the Reverse Shock
• Direct measurement of ISM proper motion with image registration
• ULISSE: Determination of star-formation rate and stellar mass based on the one-shot galaxy imaging technique
• Environmental Invariance of the Galaxy Size-Mass Relation
• Measuring the evolution of stellar bars with the host galaxy's spin
• MIGHTEE: The dark matter haloes, duty cycle and mechanical feedback from radio-AGN up to $z\sim 2.5$
• Euclid: Discovery of 31 new quasars at $6.6<z<7.8$
• Challenges to the cosmological constant model following results from the Dark Energy Survey
• Dark Energy After DESI DR2: Observational Status, Reconstructions, and Physical Models
• Neutrino mass limits and decaying dark matter: background evolution versus perturbations
• Towards an optimal extraction of cosmological parameters from galaxy cluster surveys using convolutional neural networks
• The kinematic cosmic dipole beyond Ellis and Baldwin
• Gaia serial CTI modelling and radiation damage study
• Improved Identification of Strongly Lensed Gravitational Waves with Host Galaxy Locations
• Illuminating the Dark Sector: Understanding Modified Gravity Signatures with Cross-Correlations of Gravitational Waves and Large-Scale Structure
• Flexible Simulation Based Inference for Galaxy Photometric Fitting with Synthesizer
• QUEST (Quasar Unsupervised Encoder and Synthesis Tool): A machine learning framework to generate quasar spectra
• Euclid: Exploring observational systematics in cluster cosmology -- a comprehensive analysis of cluster counts and clustering
• Using Strong Lensing to Detect Subhalos with Steep Inner Density Profiles
• Synergy between CSST and third-generation gravitational-wave detectors: Inferring cosmological parameters using cross-correlation of dark sirens and galaxies
• Parametric strong lensing model of the galaxy cluster Abell 2390 from Euclid and MUSE observations
• SHAPE. I. A SOM-SED hybrid approach for efficient galaxy parameter estimation leveraging JWST
• STRAWBERRY: Finding haloes in the gravitational potential
• Far-infrared lines hidden in archival deep multi-wavelength surveys: Limits on [CII]-158$\mu$m at $z\sim 0.3-2.9$
• The intragroup light in KiDS+GAMA groups: A stacking analysis
• The Impact of Spectroscopic Redshift Errors on Cosmological Measurements
• Stable Islands of Weak Gravity
• Strong gravitational lensing effects of black holes with quantum hair
• Measuring the IGM correlation length at 5<z<6.1: a fast change at the end of Reionization
• The miniJPAS survey quasar selection V: combined algorithm
• Forecast constraints on null tests of the $\Lambda$CDM model with SPHEREx
• Dark energy constraints in light of theoretical priors
• Angular correlation functions of bright Lyman-break galaxies at $3\lesssim \mathbf{z}\lesssim 5$
• DELVE-ing into the Milky Way's Globular Clusters: Assessing extra-tidal features in NGC 5897, NGC 7492, and testing detectability with deeper photometry
• CosmoGLINT: Cosmological Generative Model for Line Intensity Mapping with Transformer
• Denoising weak lensing mass maps with diffusion model: systematic comparison with generative adversarial network
• Dark Matter and Galaxy Cross-Correlations with the Cherenkov Telescope Array Observatory
• Identifying Astrophysical Anomalies in 99.6 Million Cutouts from the Hubble Legacy Archive Using AnomalyMatch
• Mapping neutral islands during end stages of reionization with photometric intergalactic medium tomography
• Confirming HSC strong lens candidates with DESI Spectroscopy. I. Project overview and first results
• Individual halo bias in models of $f(R)$ gravity
• Time-reversed Stochastic Inflation
• Constraining the [CII] luminosity function from the power spectrum of line-intensity maps at redshift 3.6
• Clustering of the extreme: A theoretical description of weak lensing critical points power spectra in the mildly nonlinear regime
• AMICO-WL: an optimal filtering algorithm for galaxy cluster detections with weak lensing
• Influence of photometric galaxies redshift distribution in BAO estimation
• Measuring the Stellar-to-Halo Mass Relation at $\sim 10^{10}$ Solar masses, using forthcoming space-based imaging of galaxy-galaxy strong lenses
• Constraint on Neutrino Statistics from Cosmological Data
• Toward a universal characterization methodology for conversion gain measurement of CMOS APS: application to Euclid and SVOM
• Galaxy-Point Spread Function correlations as a probe of weak-lensing systematics with UNIONS data
• The multi-dimensional halo assembly bias can be preserved when enhancing halo properties with HALOSCOPE
• Neural Networks for cosmological model selection and feature importance using Cosmic Microwave Background data
• Euclid preparation. L. Calibration of the linear halo bias in $\Lambda (\nu )$CDM cosmologies
• Modeling and measuring the anisotropic halo 3-point correlation function: a coordinated study
• Cosmic curl -- Features and convergence of the vorticity power spectrum in $N$-body simulations
• Euclid preparation: The NISP spectroscopy channel, on ground performance and calibration
• Euclid: Optimising tomographic redshift binning for 3$\times$2pt power spectrum constraints on dark energy
• The Drivers of the Decline in Supermassive Black Hole Growth at $z<2$
• Squared-field cross-correlation between kinetic Sunyaev-Zel'dovich effect and 21-cm intensity mapping
• Anisotropic Counts-in-Cells in Redshift Space: A New Route to Cosmological Constraints from Galaxy Surveys
• FuGa3D: Fast full-sky analysis of Galaxy catalogs in 3D
• Prospects for radio weak lensing: studies using LOFAR observations in the ELAIS-N1 field
• A catalog of near-IR absolute magnitudes of Solar System small bodies
• Estimating the heterogeneity of pressure profiles within a complete sample of 55 galaxy clusters: a Bayesian Hierarchical Model
• Euclid preparation. Full-shape modelling of 2-point and 3-point correlation functions in real space
• Blowing Star Formation Away in AGN Hosts (BAH) -- III. Serendipitous discovery of a $z\sim 2.9$ star-forming galaxy lensed by the galactic bulge of CGCG 012-070 using JWST NIRSpec
• A gradient boosting and broadband approach to finding Lyman-α emitting galaxies beyond narrowband surveys
• AutoKnots: Adaptive Knot Allocation for Spline Interpolation
• How to embed any likelihood into SBI: Application to Planck + Stage IV galaxy surveys and Dynamical Dark Energy
• Improving Optical Photo-z Constraints for Dusty Star-forming Galaxies Using Submillimeter-based Priors
• Structural evolution of quiescent galaxies at intermediate redshifts at UV and red rest-frame wavelengths
• Diagnosing Systematic Effects Using the Inferred Initial Power Spectrum
• Primordial non-Gaussianity systematics from redshift mismatch with SPHEREx
• From Redshift to Real Space: Combining Linear Theory With Neural Networks
• Emulating redshift mixing due to blending in weak gravitational lensing
• Euclid: Early Release Observations. Weak gravitational lensing analysis of Abell 2390
• Cosmological Analysis with Calibrated Neural Quantile Estimation and Approximate Simulators
• Incorporating curved geometry in cosmological simulations
• Web-Halo Model (WHM): Accurate non-linear matter power spectrum predictions without free parameters
• Tracing Signatures of Modified Gravity in Redshift-Space Galaxy Bispectrum Multipoles: Prospects for Euclid
• Detecting Local and Integrated Relativistic Effects by Multi-Tracing a Single Galaxy Population in Harmonic Space
• Phantom Crossing with Quintom Models
• Probing the Cosmological Principle with CMB lensing and cosmic shear
• Searching for Dark Structures: A Comparison of Weak-lensing Convergence Maps and Lensing-weighted Galaxy Density Maps
• Multi-messenger lensing time delay as a probe of the graviton mass
• Clustering analysis of medium-band selected high-redshift galaxies
• A revisited Correction to the Halo Mass Function for local-type Primordial non-Gaussianity
• Towards an application of fourth-order shear statistics I. The information content of $⟨M_{\mathrm{ap}}^4⟩$
• Enhancing Cosmological Constraints by Two-dimensional $\beta$-cosmic-web Weighted Angular Correlation Functions
• The SRG/eROSITA All-Sky Survey $J$-Band Follow-Up Observations for Selected High-Redshift Galaxy Cluster Candidates
• A Pearl in the Shell: an ultra-compact dwarf within the tidal debris surrounding spiral galaxy NGC 7531
• Performance of the image persistence model for Euclid infrared detectors
• Euclid preparation. Predicting star-forming galaxy scaling relations with the spectral stacking code SpectraPyle
• Euclid: Discovery of bright $z\simeq 7$ Lyman-break galaxies in UltraVISTA and Euclid COSMOS
• Breaking the degeneracy in stellar spectral classification from single wide-band images
• Implications of a high growth index on the variation of $G$
• Cosmological Implications of Thermodynamic Split Conjecture
• Aletheia: Emulating the non-linear matter power spectrum in the context of evolution mapping
• Euclid Structural-Thermal-Optical Performance
• Reconstructing spatially-varying multiplicative bias for Stage IV weak lensing galaxy surveys with a quadratic estimator
• The Next Generation Fornax Survey (NGFS).VIII. A Support Vector Machine Approach for Disentangling Globular Clusters from other Sources
• Identification of gravitational lenses obscured by foreground light in the KiDS dataset using U-Nets and ResNets
• Future Dark Energy Constraints from Atomic Clocks
• Integrated Sachs-Wolfe maps from the Gower Street $w$CDM simulations
• Three-point intrinsic alignments of galaxies and haloes in the FLAMINGO simulations
• Large-scale Modeling of the Observed Power Spectrum Multipoles
• Direct Detection of Type II-P Supernova Progenitors with the $\text{Euclid}$ and CSST Surveys
• Euclid: Improving redshift distribution reconstruction using a deep-to-wide transfer function
• Euclid preparation. 3D reconstruction of the cosmic web with simulated Euclid Deep spectroscopic samples
• Weak Lensing Low Multipoles
• AMICO galaxy clusters in KiDS-1000: Splashback radius from weak lensing and cluster-galaxy correlation function
• Dynamic Zoom Simulations of structure formation beyond standard cosmology
• Dwarf Galaxy Number Counts within 25 Mpc: Predictions from Local Group Analogues in TNG50
• A Quantum Genetic Algorithm with application to Cosmological Parameters Estimation
• A Non-parametric Method for the Inference of Halo Occupation Distributions
• Cluster gravitational redshifts: uncertainties and survey requirements
• D${}_4$CNN$\times$AnaCal: Physics-Informed Machine Learning for Accurate and Precise Weak Lensing Shear Estimation
• Perturbative and numerical study of nonlinear relativistic effects in weak lensing
• Dark Matter Recoupling
• Multi-scale weak lensing detection of galaxy clusters with source redshift tomography
• AGILE: an end-to-end Rubin-LSST simulation of AGNs, galaxies, and stars I. Software description and first data release
• Charge diffusion and modulation transfer function in a Nancy Grace Roman Space Telescope detector
• Ray-traced weak lensing convergence in screened modified gravity theories
• Euclid: A blue galaxy population and a brightest cluster galaxy in the making in a $z\sim 1.74$ MaDCoWS2 galaxy cluster candidate
• No Stream Left Unscathed: The imprint of a host galaxy
• The Manticore Project II: Bayesian digital twins of cosmic structure across the SDSS and BOSS volumes
• Testing string theory with combined cosmological probes: a case study for dark matter gravitons
• Cosmic Acceleration from Nothing
• Cross-correlations between X-ray clusters and the general galaxy population
• Benchmarking field-level cosmological inference from galaxy redshift surveys
• DeepVoid: A Deep Learning Void Detector
• Revising Indirect Dark Matter Constraints with Updated Astrophysical $J$-Factor Priors
• Excess of substructure due to primordial black holes
• DUCA: Dynamic Universe Cosmological Analysis. II. The impact of clustering dark energy on the halo mass function
• GalSBI-SPS: a stellar population synthesis-based galaxy population model for cosmology and galaxy evolution applications
• Identifying lopsidedness in spiral galaxies using a Deep Convolutional Neural Network
• Probing dipolar power asymmetry with galaxy clustering and intrinsic alignments
• Estimating the completeness of the QUBRICS Survey with 3501 QSO redshifts from Gaia DR3 spectra