Euclid Imaging Consortium Science Book
arXiv:1001.0061
Abstract
The energy density of the Universe is dominated by dark energy and dark matter, two mysterious components which pose some of the most important questions in fundamental science today. Euclid is a high-precision survey mission designed to answer these questions by mapping the geometry of the dark Universe. Euclid's Visible-NIR imaging and spectroscopy of the entire extragalactic sky will further produce extensive legacy science for various fields of astronomy. Over the 2008-2009 period, Euclid has been the object of an ESA Assessment Phase in which the study of the Euclid Imaging instrument was under the responsibility of the Euclid Imaging Consortium (EIC). The EIC Science Book presents the studies done by the EIC science working groups in the context of this study phase. We first give a brief description of the Euclid mission and of the imaging instrument and surveys. We then summarise the primary and legacy science which will be achieved with the Euclid imaging surveys, along with the simulations and data handling scheme which have been developed to optimise the instrument and ensure its science performance.
214 Latex pages, including full list of authors on page 3. Full resolution document available at http://www.euclid-imaging.net
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- Higgs-Dilaton Cosmology: From the Early to the Late Universe
- Titans of the Early Universe: The Prato Statement on the Origin of the First Supermassive Black Holes
- Galaxy alignments: Observations and impact on cosmology
- Probing the theory of gravity with gravitational lensing of gravitational waves and galaxy surveys
- Cosmology constraints from shear peak statistics in Dark Energy Survey Science Verification data
- Non-parametric spatial curvature inference using late-universe cosmological probes
- The Mira-Titan Universe: Precision Predictions for Dark Energy Surveys
- Cosmic shear covariance: The log-normal approximation
- Testing the general theory of relativity using gravitational wave propagation from dark standard sirens
- Quantifying Environmental and Line-of-Sight Effects in Models of Strong Gravitational Lens Systems
- The growth of density perturbations in the last 10 billion years from tomographic large-scale structure data
- preparation: XV. Forecasting cosmological constraints for the and CMB joint analysis
- Mining for Dark Matter Substructure: Inferring subhalo population properties from strong lenses with machine learning
- A General Study of the Influence of Catastrophic Photometric Redshift Errors on Cosmology with Cosmic Shear Tomography
- General Requirements on Matter Power Spectrum Predictions for Cosmology with Weak Lensing Tomography
- Time-dependence of the astrophysical stochastic gravitational wave background
- VIS: the visible imager for Euclid
- CLASH: Accurate Photometric Redshifts with 14 HST bands in Massive Galaxy Cluster Cores
- 3D Photometric Cosmic Shear
- Detectability of extrasolar moons as gravitational microlenses
- Bayesian inference from photometric redshift surveys
- Simulations of Wide-Field Weak Lensing Surveys II: Covariance Matrix of Real Space Correlation Functions
- Clustering and redshift-space distortions in interacting dark energy cosmologies
- Deblending galaxies with Variational Autoencoders: a joint multi-band, multi-instrument approach
- Constraining warm dark matter with cosmic shear power spectra
- Cluster Bulleticity
- Cosmological test of gravity using weak lensing voids
- Lyman-α Forest and Cosmic Weak Lensing in a Warm Dark Matter Universe
- Differentiable Strong Lensing: Uniting Gravity and Neural Nets through Differentiable Probabilistic Programming
- Measuring galaxy cluster masses with CMB lensing using a Maximum Likelihood estimator: Statistical and systematic error budgets for future experiments
- Tomographic weak lensing shear spectra from large N-body and hydrodynamical simulations
- BAO cosmography
- How cosmological merger histories shape the diversity of stellar haloes
- The first analytical expression to estimate photometric redshifts suggested by a machine
- Assessing the photometric redshift precision of the S-PLUS survey: the Stripe-82 as a test-case
- Breaking the Vainshtein screening in clusters of galaxies
- Non-linear weak lensing forecasts
- Modified Gravity: the CMB, Weak Lensing and General Parameterisations
- VIS: the visible imager for Euclid
- What do cluster counts really tell us about the Universe?
- Tomography from the Next Generation of Cosmic Shear Experiments for Viable f(R) Models
- Tension between SN and BAO: current status and future forecasts
- Is the baryon acoustic oscillation peak a cosmological standard ruler?
- Eigengalaxies: describing galaxy morphology using principal components in image space
- Galaxy-Galaxy Weak Lensing Measurements from SDSS: I. Image Processing and Lensing signals
- Biases on cosmological parameters by general relativity effects
- Model Independent Tests of Cosmic Gravity
- Path Integral Marginalization for Cosmology: Scale Dependent Galaxy Bias & Intrinsic Alignments
- The self similarity of weak lensing peaks
- The S-PLUS: a star/galaxy classification based on a Machine Learning approach
- On Mitigation of the Uncertainty in Nonlinear Matter Clustering for Cosmic Shear Tomography
- Figures of Merit for Testing Standard Models: Application to Dark Energy Experiments in Cosmology
- Non-Gaussian Shape Discrimination with Spectroscopic Galaxy Surveys
- Deep redshift topological lensing: strategies for the T^3 candidate
- Testing a Phenomenologically Extended DGP Model with Upcoming Weak Lensing Surveys
- High-precision spectra for dynamical Dark Energy cosmologies from constant-w models
- Constraining Ultra-light Axions with Galaxy Cluster Number Counts
- Beyond the Standard Model of Physics with Astronomical Observations
- Large Scale Searches for Brown Dwarfs and Free-Floating Planets
- Cosmic flexion
- Testing the Origin of the CMB Large-Angle Correlation Deficit with a Galaxy Imaging Survey
- Using gamma regression for photometric redshifts of survey galaxies
- Strong lensing cross sections for isothermal models - I. Finite source effects in the circular case
- Analytic Derivation of the Halo Mass Function from the Non-Linear Cosmic Density Field
- Morphological classification of astronomical images with limited labelling
- Redshift-space galaxy bispectrum in presence of massive neutrinos: A multipole expansion approach for Euclid
- Comparison of Graphcore IPUs and Nvidia GPUsfor cosmology applications