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Euclid Imaging Consortium Science Book
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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.
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Cited by 5 Pith papers
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Mining for Dark Matter Substructure: Inferring subhalo population properties from strong lenses with machine learning
A neural likelihood ratio estimator trained on simulated strong lensing images can infer the abundance and mass slope of dark matter subhalos from an ensemble of lenses.
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Probing the theory of gravity with gravitational lensing of gravitational waves and galaxy surveys
Cross-correlating gravitational wave lensing with galaxy surveys is forecast to detect weak lensing of gravitational waves at z<0.5 within about 10 years, with black hole-neutron star mergers as the most promising source.
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Multi-messenger tests of gravity with weakly lensed gravitational waves
The authors show that cross-correlating GW source convergence with CMB lensing can measure a GR prediction (identical geodesics for GWs and photons) at high SNR for LISA-class detectors.
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Multi-Messenger Cosmology: A Route to Accurate Inference of Dark Energy Beyond CPL Parametrization from XG Detectors
A simulation forecast claims CE+ET bright standard sirens can measure dark energy EoS parameters with sigma(w0)=0.010, sigma(wa)=0.049, sigma(wb)=0.072, better than other planned probes.
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A new probe of Axion-Like Particles: CMB polarization distortions due to cluster magnetic fields
Resonant photon-to-axion conversion in galaxy cluster magnetic fields creates a polarized CMB distortion that future experiments could use to constrain ALP couplings two orders of magnitude better than current bounds.
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