The Euclid mission design
Giuseppe D Racca, Rene Laureijs, Luca Stagnaro, Jean Christophe, Salvignol, Jose Lorenzo Alvarez, Gonzalo Saavedra Criado, Luis Gaspar, Venancio, Alex Short, Paolo Strada, Tobias Boenke, Cyril Colombo, Adriano, Calvi, Elena Maiorano, Osvaldo Piersanti, Sylvain Prezelus

TL;DR
Euclid is a space mission by ESA designed to study dark energy, dark matter, and gravity through optical and near-infrared surveys, utilizing weak lensing and galaxy clustering over a large portion of the sky.
Contribution
This paper details the design and instrumentation of the Euclid mission, including its spacecraft, telescope, and survey strategy, aimed at cosmological research.
Findings
Mission scheduled for launch in 2020 with 6 years of operation.
Survey will cover more than 35% of the sky.
Instruments include a 1.2 m telescope, visible imager, and near-infrared spectro-photometer.
Abstract
Euclid is a space-based optical/near-infrared survey mission of the European Space Agency (ESA) to investigate the nature of dark energy, dark matter and gravity by observing the geometry of the Universe and on the formation of structures over cosmological timescales. Euclid will use two probes of the signature of dark matter and energy: Weak gravitational Lensing, which requires the measurement of the shape and photometric redshifts of distant galaxies, and Galaxy Clustering, based on the measurement of the 3-dimensional distribution of galaxies through their spectroscopic redshifts. The mission is scheduled for launch in 2020 and is designed for 6 years of nominal survey operations. The Euclid Spacecraft is composed of a Service Module and a Payload Module. The Service Module comprises all the conventional spacecraft subsystems, the instruments warm electronics units, the sun shield…
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