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Title:
The Euclid Data Processing Challenges
Authors:
Dubath, Pierre; Apostolakos, Nikolaos; Bonchi, Andrea; Belikov, Andrey; Brescia, Massimo; Cavuoti, Stefano; Capak, Peter; Coupon, Jean; Dabin, Christophe; Degaudenzi, Hubert; Desai, Shantanu; Dubath, Florian; Fontana, Adriano; Fotopoulou, Sotiria; Frailis, Marco; Galametz, Audrey; Hoar, John; Holliman, Mark; Hoyle, Ben; Hudelot, Patrick; Ilbert, Olivier; Kuemmel, Martin; Melchior, Martin; Mellier, Yannick; Mohr, Joe; Morisset, Nicolas; Paltani, Stéphane; Pello, Roser; Pilo, Stefano; Polenta, Gianluca; Poncet, Maurice; Saglia, Roberto; Salvato, Mara; Sauvage, Marc; Schefer, Marc; Serrano, Santiago; Soldati, Marco; Tramacere, Andrea; Williams, Rees; Zacchei, Andrea
Affiliation:
AA( Department of Astronomy, University of Geneva, Switzerland ), AB( Department of Astronomy, University of Geneva, Switzerland ), AC( ASI Science Data Center, Roma, Italy), AD( Kapteyn Astronomical Institute, University of Groningen, the Netherlands), AE( INAF, Astronomical Observatory of Capodimonte, Napoli, Italy), AF( INAF, Astronomical Observatory of Capodimonte, Napoli, Italy), AG( California Institute of Technology, Infrared Processing and Analysis Center, Pasadena, USA), AH( Department of Astronomy, University of Geneva, Switzerland ), AI( Centre National d'Études Spatiales, Toulouse, France), AJ( Department of Astronomy, University of Geneva, Switzerland ), AK( Department of Physics, IIT Hyderabad, Kandi, India), AL( Department of Astronomy, University of Geneva, Switzerland ), AM( INAF, Osservatorio Astronomico di Roma, Monte Porzio Catone, Italy), AN( Department of Astronomy, University of Geneva, Switzerland ), AO( INAF - Osservatorio Astronomico di Trieste, Italy), AP( MPE, Max-Planck-Institut für Extraterrestrische Physik, Garching, Germany), AQ( European Space Astronomy Centre, European Space Agency, Madrid, Spain), AR( Institute for Astronomy, University of Edinburgh), AS( MPE, Max-Planck-Institut für Extraterrestrische Physik, Garching, Germany), AT( CNRS-UPMC, Institut d'Astrophysique de Paris, France), AU( Aix Marseille Univ, CNRS, Laboratoire d'Astrophysique de Marseille (LAM), France), AV( Fakultät fr Physik, Ludwig-Maximilians-Universität, München, Germany), AW( Fachhochschule Nordwestschweiz, Institute of 4D Technologies, Windisch, Switzerland), AX( CNRS-UPMC, Institut d'Astrophysique de Paris, France), AY( Fakultät fr Physik, Ludwig-Maximilians-Universität, München, Germany), AZ( Department of Astronomy, University of Geneva, Switzerland ), BA( Department of Astronomy, University of Geneva, Switzerland ), BB( Université de Toulouse, UPS-OMP, CNRS, IRAP, France), BC( INAF, Osservatorio Astronomico di Roma, Monte Porzio Catone, Italy), BD( ASI Science Data Center, Roma, Italy), BE( Centre National d'Études Spatiales, Toulouse, France), BF( MPE, Max-Planck-Institut für Extraterrestrische Physik, Garching, Germany), BG( MPE, Max-Planck-Institut für Extraterrestrische Physik, Garching, Germany), BH( Laboratoire AIM Paris-Saclay, CEA/IRFU/SAp, CNRS, Universite Paris Diderot, France), BI( Department of Astronomy, University of Geneva, Switzerland ), BJ( Institute of Space Sciences (IEEC-CSIC), Campus UAB, Barcelona, Spain), BK( Fachhochschule Nordwestschweiz, Institute of 4D Technologies, Windisch, Switzerland), BL( Department of Astronomy, University of Geneva, Switzerland ), BM( Center of Information Technology, University of Groningen, the Netherlands), BN( INAF - Osservatorio Astronomico di Trieste, Italy)
Publication:
Astroinformatics, Proceedings of the International Astronomical Union, IAU Symposium, Volume 325, pp. 73-82
Publication Date:
06/2017
Origin:
CUP
Keywords:
dark matter, galaxies: distances and redshifts, galaxies: fundamental parameters, surveys, catalogs, methods: data analysis,
Abstract Copyright:
(c) 2017: Copyright © International Astronomical Union 2017
DOI:
10.1017/S1743921317001521
Bibliographic Code:
2017IAUS..325...73D

Abstract

Euclid is a Europe-led cosmology space mission dedicated to a visible and near infrared survey of the entire extra-galactic sky. Its purpose is to deepen our knowledge of the dark content of our Universe. After an overview of the Euclid mission and science, this contribution describes how the community is getting organized to face the data analysis challenges, both in software development and in operational data processing matters. It ends with a more specific account of some of the main contributions of the Swiss Science Data Center (SDC-CH).
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