Euclid. I. Overview of the Euclid mission

Euclid. I. Overview of the Euclid mission

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 provi...

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Veröffentlicht in:arXiv.org 2024-09
Hauptverfasser: Adam, R, Addison, G E, Allevato, V, Azzollini, R, Bardelli, S, Barthelemy, A, Battisti, A J, Bazzanini, L, Belikov, A N, Benabed, K, Benson, K, Bethermin, M, Bhargava, S, Bolzonella, M, Brau-Nogue, S, Brekke, P, Caillat, A, Casey, C M, Cassata, P, Castelao, D, Charles, Y, Chartab, N, Colbert, J, Costille, A, Courtois, H M, Cowell, T, D'Amico, G, Dannerbauer, H, Da Silva, A, Doumerg, W d'Assignies, de la Torre, S, Denniston, J, De Petris, M, Durrer, R, Faustini, F, Ferriol, S, Fouchez, D, Fourmanoit, N, Gabarra, L, Ganga, K, Gwyn, S, Haase, J, Helou, G, Henares, K, Hernández-Monteagudo, C, Hoekstra, H, Holmes, W, Hook, I, Israelsson, U E, Jahnke, K, Kovačić, I, Lahav, O, Langer, M, Laudisio, F, Q Le Boulc'h, Levi, M E, Maino, D, Maiorano, E, Meylan, G, Montoro, A, Moresco, M, Moscardini, L, Murray, C, Nagam, B C, Navarro-Alsina, A, Nesseris, S, Noller, J, Nutma, T, Oppizzi, F, Parimbelli, G, Paterson, K, Plana, C, Popa, V, Poulain, M, Reimberg, P, Rudolph, A, Rusholme, B, Saponara, M, Schmidt, M, Schneider, P, Shuntov, M, Silvestri, A, Slezak, E, Smith, R E, Soldano, F, Stanco, L, Stern, D, Tao, C, Tavagnacco, D, Thizy, C, Urbano, M, Valieri, C, Ventura, S, Kleijn, G Verdoes, Verma, A, Viitanen, A, Widmer, A, Yankelevich, V, Zalesky, L, Zerbi, F M
Format: Artikel
Sprache:eng
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Astronomical models
Clustering
Cosmology
Dark energy
Dark matter
Data processing
Image resolution
Infrared imaging
Near infrared radiation
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creator Adam, R
Addison, G E
Allevato, V
Azzollini, R
Bardelli, S
Barthelemy, A
Battisti, A J
Bazzanini, L
Belikov, A N
Benabed, K
Benson, K
Bethermin, M
Bhargava, S
Bolzonella, M
Brau-Nogue, S
Brekke, P
Caillat, A
Casey, C M
Cassata, P
Castelao, D
Charles, Y
Chartab, N
Colbert, J
Costille, A
Courtois, H M
Cowell, T
D'Amico, G
Dannerbauer, H
Da Silva, A
Doumerg, W d'Assignies
de la Torre, S
Denniston, J
De Petris, M
Durrer, R
Faustini, F
Ferriol, S
Fouchez, D
Fourmanoit, N
Gabarra, L
Ganga, K
Gwyn, S
Haase, J
Helou, G
Henares, K
Hernández-Monteagudo, C
Hoekstra, H
Holmes, W
Hook, I
Israelsson, U E
Jahnke, K
Kovačić, I
Lahav, O
Langer, M
Laudisio, F
Q Le Boulc'h
Levi, M E
Maino, D
Maiorano, E
Meylan, G
Montoro, A
Moresco, M
Moscardini, L
Murray, C
Nagam, B C
Navarro-Alsina, A
Nesseris, S
Noller, J
Nutma, T
Oppizzi, F
Parimbelli, G
Paterson, K
Plana, C
Popa, V
Poulain, M
Reimberg, P
Rudolph, A
Rusholme, B
Saponara, M
Schmidt, M
Schneider, P
Shuntov, M
Silvestri, A
Slezak, E
Smith, R E
Soldano, F
Stanco, L
Stern, D
Tao, C
Tavagnacco, D
Thizy, C
Urbano, M
Valieri, C
Ventura, S
Kleijn, G Verdoes
Verma, A
Viitanen, A
Widmer, A
Yankelevich, V
Zalesky, L
Zerbi, F M
description 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.
format Article
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I. Overview of the Euclid mission</title><title>arXiv.org</title><description>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.</description><subject>Astronomical models</subject><subject>Clustering</subject><subject>Cosmology</subject><subject>Dark energy</subject><subject>Dark matter</subject><subject>Data processing</subject><subject>Image resolution</subject><subject>Infrared imaging</subject><subject>Near infrared radiation</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2024</creationdate><recordtype>article</recordtype><sourceid>ABUWG</sourceid><sourceid>AFKRA</sourceid><sourceid>AZQEC</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><recordid>eNpjYuA0MjY21LUwMTLiYOAtLs4yMDAwMjM3MjU15mTQdC1NzslM0VPw1FPwL0stKstMLVfIT1MoyUhVgEgp5GYWF2fm5_EwsKYl5hSn8kJpbgZlN9cQZw_dgqL8wtLU4pL4rPzSojygVLyxgamlmZGJhaWBMXGqAGR1L4o</recordid><startdate>20240924</startdate><enddate>20240924</enddate><creator>Adam, R</creator><creator>Addison, G E</creator><creator>Allevato, V</creator><creator>Azzollini, R</creator><creator>Bardelli, S</creator><creator>Barthelemy, A</creator><creator>Battisti, A J</creator><creator>Bazzanini, L</creator><creator>Belikov, A N</creator><creator>Benabed, K</creator><creator>Benson, K</creator><creator>Bethermin, M</creator><creator>Bhargava, S</creator><creator>Bolzonella, M</creator><creator>Brau-Nogue, S</creator><creator>Brekke, P</creator><creator>Caillat, A</creator><creator>Casey, C M</creator><creator>Cassata, P</creator><creator>Castelao, D</creator><creator>Charles, Y</creator><creator>Chartab, N</creator><creator>Colbert, J</creator><creator>Costille, A</creator><creator>Courtois, H M</creator><creator>Cowell, T</creator><creator>D'Amico, G</creator><creator>Dannerbauer, H</creator><creator>Da Silva, A</creator><creator>Doumerg, W d'Assignies</creator><creator>de la Torre, S</creator><creator>Denniston, J</creator><creator>De Petris, M</creator><creator>Durrer, R</creator><creator>Faustini, F</creator><creator>Ferriol, S</creator><creator>Fouchez, D</creator><creator>Fourmanoit, N</creator><creator>Gabarra, L</creator><creator>Ganga, K</creator><creator>Gwyn, S</creator><creator>Haase, J</creator><creator>Helou, G</creator><creator>Henares, K</creator><creator>Hernández-Monteagudo, C</creator><creator>Hoekstra, H</creator><creator>Holmes, W</creator><creator>Hook, I</creator><creator>Israelsson, U E</creator><creator>Jahnke, K</creator><creator>Kovačić, I</creator><creator>Lahav, O</creator><creator>Langer, M</creator><creator>Laudisio, F</creator><creator>Q Le Boulc'h</creator><creator>Levi, M E</creator><creator>Maino, D</creator><creator>Maiorano, E</creator><creator>Meylan, G</creator><creator>Montoro, A</creator><creator>Moresco, M</creator><creator>Moscardini, L</creator><creator>Murray, C</creator><creator>Nagam, B C</creator><creator>Navarro-Alsina, A</creator><creator>Nesseris, S</creator><creator>Noller, J</creator><creator>Nutma, T</creator><creator>Oppizzi, F</creator><creator>Parimbelli, G</creator><creator>Paterson, K</creator><creator>Plana, C</creator><creator>Popa, V</creator><creator>Poulain, M</creator><creator>Reimberg, P</creator><creator>Rudolph, A</creator><creator>Rusholme, B</creator><creator>Saponara, M</creator><creator>Schmidt, M</creator><creator>Schneider, P</creator><creator>Shuntov, M</creator><creator>Silvestri, A</creator><creator>Slezak, E</creator><creator>Smith, R E</creator><creator>Soldano, F</creator><creator>Stanco, L</creator><creator>Stern, D</creator><creator>Tao, C</creator><creator>Tavagnacco, D</creator><creator>Thizy, C</creator><creator>Urbano, M</creator><creator>Valieri, C</creator><creator>Ventura, S</creator><creator>Kleijn, G Verdoes</creator><creator>Verma, A</creator><creator>Viitanen, A</creator><creator>Widmer, A</creator><creator>Yankelevich, V</creator><creator>Zalesky, L</creator><creator>Zerbi, F M</creator><general>Cornell University Library, arXiv.org</general><scope>8FE</scope><scope>8FG</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>L6V</scope><scope>M7S</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>PTHSS</scope></search><sort><creationdate>20240924</creationdate><title>Euclid. I. Overview of the Euclid mission</title><author>Adam, R ; Addison, G E ; Allevato, V ; Azzollini, R ; Bardelli, S ; Barthelemy, A ; Battisti, A J ; Bazzanini, L ; Belikov, A N ; Benabed, K ; Benson, K ; Bethermin, M ; Bhargava, S ; Bolzonella, M ; Brau-Nogue, S ; Brekke, P ; Caillat, A ; Casey, C M ; Cassata, P ; Castelao, D ; Charles, Y ; Chartab, N ; Colbert, J ; Costille, A ; Courtois, H M ; Cowell, T ; D'Amico, G ; Dannerbauer, H ; Da Silva, A ; Doumerg, W d'Assignies ; de la Torre, S ; Denniston, J ; De Petris, M ; Durrer, R ; Faustini, F ; Ferriol, S ; Fouchez, D ; Fourmanoit, N ; Gabarra, L ; Ganga, K ; Gwyn, S ; Haase, J ; Helou, G ; Henares, K ; Hernández-Monteagudo, C ; Hoekstra, H ; Holmes, W ; Hook, I ; Israelsson, U E ; Jahnke, K ; Kovačić, I ; Lahav, O ; Langer, M ; Laudisio, F ; Q Le Boulc'h ; Levi, M E ; Maino, D ; Maiorano, E ; Meylan, G ; Montoro, A ; Moresco, M ; Moscardini, L ; Murray, C ; Nagam, B C ; Navarro-Alsina, A ; Nesseris, S ; Noller, J ; Nutma, T ; Oppizzi, F ; Parimbelli, G ; Paterson, K ; Plana, C ; Popa, V ; Poulain, M ; Reimberg, P ; Rudolph, A ; Rusholme, B ; Saponara, M ; Schmidt, M ; Schneider, P ; Shuntov, M ; Silvestri, A ; Slezak, E ; Smith, R E ; Soldano, F ; Stanco, L ; Stern, D ; Tao, C ; Tavagnacco, D ; Thizy, C ; Urbano, M ; Valieri, C ; Ventura, S ; Kleijn, G Verdoes ; Verma, A ; Viitanen, A ; Widmer, A ; Yankelevich, V ; Zalesky, L ; Zerbi, F M</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-proquest_journals_30596248903</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2024</creationdate><topic>Astronomical models</topic><topic>Clustering</topic><topic>Cosmology</topic><topic>Dark energy</topic><topic>Dark matter</topic><topic>Data processing</topic><topic>Image resolution</topic><topic>Infrared imaging</topic><topic>Near infrared radiation</topic><toplevel>online_resources</toplevel><creatorcontrib>Adam, 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Collection</collection><collection>ProQuest Engineering Collection</collection><collection>Engineering Database</collection><collection>Access via ProQuest (Open Access)</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><collection>Engineering Collection</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Adam, R</au><au>Addison, G E</au><au>Allevato, V</au><au>Azzollini, R</au><au>Bardelli, S</au><au>Barthelemy, A</au><au>Battisti, A J</au><au>Bazzanini, L</au><au>Belikov, A N</au><au>Benabed, K</au><au>Benson, K</au><au>Bethermin, M</au><au>Bhargava, S</au><au>Bolzonella, M</au><au>Brau-Nogue, S</au><au>Brekke, P</au><au>Caillat, A</au><au>Casey, C M</au><au>Cassata, P</au><au>Castelao, D</au><au>Charles, Y</au><au>Chartab, N</au><au>Colbert, J</au><au>Costille, A</au><au>Courtois, H M</au><au>Cowell, T</au><au>D'Amico, G</au><au>Dannerbauer, H</au><au>Da Silva, A</au><au>Doumerg, W d'Assignies</au><au>de la Torre, S</au><au>Denniston, J</au><au>De Petris, M</au><au>Durrer, R</au><au>Faustini, F</au><au>Ferriol, S</au><au>Fouchez, D</au><au>Fourmanoit, N</au><au>Gabarra, L</au><au>Ganga, K</au><au>Gwyn, S</au><au>Haase, J</au><au>Helou, G</au><au>Henares, K</au><au>Hernández-Monteagudo, C</au><au>Hoekstra, H</au><au>Holmes, W</au><au>Hook, I</au><au>Israelsson, U E</au><au>Jahnke, K</au><au>Kovačić, I</au><au>Lahav, O</au><au>Langer, M</au><au>Laudisio, F</au><au>Q Le Boulc'h</au><au>Levi, M E</au><au>Maino, D</au><au>Maiorano, E</au><au>Meylan, G</au><au>Montoro, A</au><au>Moresco, M</au><au>Moscardini, L</au><au>Murray, C</au><au>Nagam, B C</au><au>Navarro-Alsina, A</au><au>Nesseris, S</au><au>Noller, J</au><au>Nutma, T</au><au>Oppizzi, F</au><au>Parimbelli, G</au><au>Paterson, K</au><au>Plana, C</au><au>Popa, V</au><au>Poulain, M</au><au>Reimberg, P</au><au>Rudolph, A</au><au>Rusholme, B</au><au>Saponara, M</au><au>Schmidt, M</au><au>Schneider, P</au><au>Shuntov, M</au><au>Silvestri, A</au><au>Slezak, E</au><au>Smith, R E</au><au>Soldano, F</au><au>Stanco, L</au><au>Stern, D</au><au>Tao, C</au><au>Tavagnacco, D</au><au>Thizy, C</au><au>Urbano, M</au><au>Valieri, C</au><au>Ventura, S</au><au>Kleijn, G Verdoes</au><au>Verma, A</au><au>Viitanen, A</au><au>Widmer, A</au><au>Yankelevich, V</au><au>Zalesky, L</au><au>Zerbi, F M</au><format>book</format><genre>document</genre><ristype>GEN</ristype><atitle>Euclid. I. Overview of the Euclid mission</atitle><jtitle>arXiv.org</jtitle><date>2024-09-24</date><risdate>2024</risdate><eissn>2331-8422</eissn><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.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><oa>free_for_read</oa></addata></record>
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identifier EISSN: 2331-8422
ispartof arXiv.org, 2024-09
issn 2331-8422
language eng
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source Freely Accessible Journals
subjects Astronomical models
Clustering
Cosmology
Dark energy
Dark matter
Data processing
Image resolution
Infrared imaging
Near infrared radiation
title Euclid. I. Overview of the Euclid mission
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