This HTML5 document contains 507 embedded RDF statements represented using HTML+Microdata notation.

The embedded RDF content will be recognized by any processor of HTML5 Microdata.

PrefixNamespace IRI
n44http://www.idref.fr/233130799/
xsdhhttp://www.w3.org/2001/XMLSchema#
n69http://www.idref.fr/235928291/
n57http://orcid.org/0000-0001-6764-073X#
n61http://orcid.org/0000-0003-4145-1943#
n76http://orcid.org/0000-0001-9110-5550#
n83http://www.idref.fr/175198462/
n23http://www.idref.fr/169030458/
vivohttp://vivoweb.org/ontology/core#
marcrelhttp://id.loc.gov/vocabulary/relators/
n9http://orcid.org/0000-0002-4749-2984#
n11http://orcid.org/0000-0001-6225-3693#
rdfhttp://www.w3.org/1999/02/22-rdf-syntax-ns#
n72http://orcid.org/0000-0002-6497-5881#
n12http://orcid.org/0000-0003-3804-2137#
n17http://orcid.org/0000-0002-6385-1609#
n80http://orcid.org/0000-0002-0644-5727#
hubhttp://hub.abes.fr/namespace/
n47http://orcid.org/0000-0001-6512-6358#
bibohttp://purl.org/ontology/bibo/
n62http://orcid.org/0000-0003-2035-9339#
n28http://orcid.org/0000-0003-1059-2532#
n45http://www.idref.fr/23545267X/
n32http://orcid.org/0000-0003-4285-9086#
n81http://orcid.org/0000-0003-1820-5998#
n36http://orcid.org/0000-0002-5845-8132#
n41http://orcid.org/0000-0003-2040-4654#
n58http://www.idref.fr/07450326X/
n16http://orcid.org/0000-0003-4172-4606#
n79http://orcid.org/0000-0001-9856-1970#
n73http://orcid.org/0000-0002-0236-919X#
n7http://orcid.org/0000-0003-0125-3563#
n40http://orcid.org/0000-0002-8850-0303#
n21http://orcid.org/0000-0002-3130-0204#
n19http://orcid.org/0000-0003-2508-0046#
n43http://hub.abes.fr/edp/periodical/articletype/
n51http://www.idref.fr/170321126/
n63http://orcid.org/0000-0002-8201-1525#
n30http://orcid.org/0000-0002-7926-3481#
n31https://www.edpsciences.
n49http://hub.abes.fr/edp/periodical/aa/2022/volume_657/issue_2022/
n59http://orcid.org/0000-0002-4823-3757#
n10http://orcid.org/0000-0003-2317-5471#
n77http://orcid.org/0000-0002-3748-5115#
n52http://orcid.org/0000-0001-6831-0687#
n13http://orcid.org/0000-0001-7020-1172#
n60http://www.idref.fr/203953622/
n2http://hub.abes.fr/edp/periodical/aa/2022/volume_657/issue_2022/aa41556-21/
n18http://www.idref.fr/224540513/
n53http://orcid.org/0000-0001-7089-4503#
n27http://orcid.org/0000-0002-3089-7846#
n56http://orcid.org/0000-0002-3309-7692#
n29http://orcid.org/0000-0001-9272-5292#
rdachttp://rdaregistry.info/Elements/c/
n50http://orcid.org/0000-0003-4444-8651#
n20http://www.idref.fr/175198330/
n22http://orcid.org/0000-0002-4537-6218#
n74http://orcid.org/0000-0002-7522-4645#
n55http://hub.abes.fr/referentiel/edparticlecategories/subject/
n66http://hub.abes.fr/edp/periodical/aa/
n84http://orcid.org/0000-0003-0396-1192#
n35http://orcid.org/0000-0002-6085-3780#
dctermshttp://purl.org/dc/terms/
n4http://hub.abes.fr/edp/periodical/aa/2022/volume_657/issue_2022/aa41556-21/authorship/
rdawhttp://rdaregistry.info/Elements/w/
n46http://orcid.org/0000-0001-9234-7412#
n67http://orcid.org/0000-0002-0211-2861#
n15http://www.idref.fr/15009728X/
n68http://orcid.org/0000-0002-8900-0298#
n78http://orcid.org/0000-0003-4067-9196#
n85http://orcid.org/0000-0001-7085-0412#
n38http://orcid.org/0000-0003-4481-3559#
n39http://orcid.org/0000-0003-3481-3491#
n34http://www.idref.fr/253830176/
n75http://orcid.org/0000-0002-0585-6591#
n82http://orcid.org/0000-0003-0238-4047#
n8http://orcid.org/0000-0003-3167-2574#
n65http://hub.abes.fr/edp/periodical/aa/2022/volume_657/issue_2022/aa41556-21/m/
n14http://orcid.org/0000-0003-1032-6680#
n6http://orcid.org/0000-0002-4618-3063#
n70http://www.idref.fr/19059568X/
n25http://hub.abes.fr/edp/periodical/aa/2022/volume_657/issue_2022/aa41556-21/subject/
n26http://orcid.org/0000-0002-1336-8328#
n71http://www.idref.fr/203078837/
n54http://www.idref.fr/241364418/
n33http://www.idref.fr/074301454/
Subject Item
n2:w
rdf:type
bibo:Article rdac:C10001
dcterms:isPartOf
n49:w
dcterms:subject
n25:surveys n25:largescalestructureofuniverse n25:methodsstatistical n55:cosmologyincludingclustersofgalaxies n25:cosmicbackgroundradiation
hub:subTitle
XV. Forecasting cosmological constraints for the Euclid and CMB joint analysis
dcterms:license
n31:org
dcterms:title
Euclid preparation
dcterms:date
2022-01-01
rdaw:P10072
n65:print n65:web
vivo:relatedBy
n4:94 n4:96 n4:92 n4:93 n4:70 n4:71 n4:52 n4:57 n4:28 n4:5 n4:208 n4:37 n4:210 n4:38 n4:33 n4:35 n4:95 n4:29 n4:98 n4:3 n4:9 n4:25 n4:91 n4:26 n4:8 n4:49 n4:83 n4:51 n4:47 n4:48 n4:44 n4:45 n4:42 n4:43 n4:61 n4:62 n4:6 n4:60 n4:56 n4:58 n4:54 n4:55 n4:77 n4:78 n4:72 n4:76 n4:69 n4:7 n4:63 n4:67 n4:125 n4:135 n4:106 n4:50 n4:65 n4:23 n4:31 n4:175 n4:197 n4:155 n4:163 n4:73 n4:110 n4:113 n4:108 n4:11 n4:102 n4:105 n4:10 n4:100 n4:169 n4:170 n4:167 n4:168 n4:162 n4:164 n4:157 n4:158 n4:183 n4:184 n4:180 n4:182 n4:179 n4:18 n4:171 n4:178 n4:199 n4:200 n4:194 n4:198 n4:191 n4:193 n4:187 n4:189 n4:22 n4:24 n4:209 n4:21 n4:206 n4:207 n4:202 n4:203 n4:121 n4:123 n4:119 n4:12 n4:116 n4:117 n4:114 n4:115 n4:132 n4:133 n4:13 n4:131 n4:128 n4:129 n4:126 n4:127 n4:142 n4:144 n4:139 n4:14 n4:137 n4:138 n4:134 n4:136 n4:154 n4:156 n4:152 n4:153 n4:15 n4:151 n4:145 n4:148 n4:32 n4:34 n4:27 n4:30 n4:195 n4:2 n4:19 n4:190 n4:53 n4:59 n4:41 n4:46 n4:4 n4:40 n4:36 n4:39 n4:89 n4:90 n4:75 n4:86 n4:68 n4:74 n4:64 n4:66 n4:124 n4:140 n4:118 n4:122 n4:107 n4:111 n4:101 n4:176 n4:185 n4:17 n4:174 n4:165 n4:166 n4:146 n4:149 n4:103 n4:104 n4:147 n4:150 n4:141 n4:143 n4:120 n4:130 n4:109 n4:112 n4:177 n4:181 n4:172 n4:173 n4:160 n4:161 n4:159 n4:16 n4:204 n4:205 n4:20 n4:201 n4:192 n4:196 n4:186 n4:188 n4:87 n4:88 n4:84 n4:85 n4:81 n4:82 n4:79 n4:80 n4:97 n4:99
marcrel:aut
n6:person n7:person n8:person n9:person n10:person n11:person n2:wenzll n2:yankelevichv n12:person n2:zamoranig n2:zoubianj n2:vassallot n13:person n2:verdoeskleijnga n14:person n2:vielzeufp n2:wellerj n15:id n2:zuccae n2:sakrz n2:sanchezag n2:schirmerm n2:schultheism n2:pettorinov n2:kohleyr n2:kurkisuonioh n2:rebolor n2:lacasaf n2:romellie n2:rossetc n2:ligoris n2:holmesw n2:tramacerea n16:person n2:hormuthf n2:tutusausi n2:valentijnea n2:kermiches n2:valiviitaj n2:kiesslinga n2:serranos n2:marullif n2:maturim n2:sirrig n17:person n2:merline n2:stancol n2:meylang n2:tentim n2:lloroi n2:maurin n2:mainettig n2:maurogordatos n2:marinuccid n2:meis n2:martinetn n2:metcalfrb n2:dubathf n2:legrandl n2:mansuttio n2:dusinis n2:marggrafo n2:farrenss n2:markovick n2:ferreirapg n2:niemism n2:corcionel n2:nightingalej n2:cropperm n2:padillac n2:dasilvaa n2:degaudenzih n2:pasianf n2:morescom n2:gillardw n18:id n19:person n2:gozaliaslg n2:moscardinil n20:id n2:gruppf n2:munarie n2:natolip n21:person n2:hoekstrah n2:flosereimbergp n2:frailism n2:galeottas n2:gangak n2:andreons n2:auricchion n2:baccigalupic n2:balagueraantolineza n2:aghanimn n2:cardonevf n22:person n2:castellanom n2:cavuotis n2:copiny n2:baldim n2:bermejoclimentjr n23:id n2:cabanacr n2:capobiancov n26:person n27:person n28:person n29:person n30:person n32:person n33:id n34:id n35:person n2:keihanene n36:person n2:kilbingerm n2:kirkpatrickcc n2:liljepb n2:gruppusoa n2:guzzol n2:hudelotp n2:jahnkek n2:medinacelie n2:meneghettim n2:neissnerc n2:ntelisp n2:lindholmv n38:person n2:mainod n2:martinellim n2:masseyr n2:castignanig n2:cledassour n2:conversil n2:diferdinandod n39:person n2:carbonec n2:carvalhocs n40:person n2:casass n41:person n2:castanderfj n2:franceschie n2:garillib n2:gillisb n2:giocolic n2:doleh n2:douspism n2:ealeta n2:finellif n2:graciacarpioj n2:graziana n2:haugansvh n2:hernandezmonteagudoc n2:farinam n2:fosalbap n2:franzettip n44:id n2:fumanam n2:kunzm n2:bozzoe n2:langerm n2:brinchmannj n2:lattanzim n2:buriganac n2:laureijsr n2:cameras n2:ilics n2:amaraa n2:kitchingt n2:bardellis n2:blancharda n2:kubikb n2:borganis n2:kummelm n45:id n2:cimattia n2:colodrocondec n2:congedog n2:conselicecj n2:branchinie n2:bresciam n2:cappia n2:carreteroj n46:person n2:delatorres n47:person n2:duncancaj n2:dupacx n2:fabbiang n2:costillea n2:couponj n2:courtoishm n2:cubyj n2:benderr n2:bivianoa n2:bodendorfc n50:person n2:boninod n2:archidiaconom n2:ballardinim n51:id n52:person n53:person n54:id n2:rossettie n2:scaramellar n2:secrouna n2:seidelg n2:paganol n2:pedersenk n2:piress n2:potterd n56:person n2:whittakerl n57:person n2:talladacrespip n2:terenoi n2:wangy n58:id n59:person n60:id n61:person n62:person n63:person n67:person n68:person n69:id n70:id n71:id n72:person n73:person n74:person n75:person n2:zaccheia n76:person n2:schneiderp n77:person n2:scottezv n2:sirignanoc n2:starckjl n2:ricciog n2:roncarellim n2:sagliar n2:saponed n2:torradeflotf n2:valenzianol n2:vielm n2:welikalan n2:sureauf n2:tayloran n2:teyssierr n2:toledomoreor n2:paltanis n2:paolettid n2:patriziil n2:percivalw n2:migliacciom n78:person n2:morganteg n2:morinb n2:nucitaaa n2:pozzettil n2:raisonf n2:renzia n2:rhodesj n2:polentag n79:person n2:poncetm n2:popal n2:pourtsidoua n80:person n81:person n82:person n83:id n84:person n85:person
dcterms:abstract
The combination and cross-correlation of the upcoming Euclid data with cosmic microwave background (CMB) measurements is a source of great expectation since it will provide the largest lever arm of epochs, ranging from recombination to structure formation across the entire past light cone. In this work, we present forecasts for the joint analysis of Euclid and CMB data on the cosmological parameters of the standard cosmological model and some of its extensions. This work expands and complements the recently published forecasts based on Euclid-specific probes, namely galaxy clustering, weak lensing, and their cross-correlation. With some assumptions on the specifications of current and future CMB experiments, the predicted constraints are obtained from both a standard Fisher formalism and a posterior-fitting approach based on actual CMB data. Compared to a Euclid-only analysis, the addition of CMB data leads to a substantial impact on constraints for all cosmological parameters of the standard Λ-cold-dark-matter model, with improvements reaching up to a factor of ten. For the parameters of extended models, which include a redshift-dependent dark energy equation of state, non-zero curvature, and a phenomenological modification of gravity, improvements can be of the order of two to three, reaching higher than ten in some cases. The results highlight the crucial importance for cosmological constraints of the combination and cross-correlation of Euclid probes with CMB data.
hub:articleType
n43:researcharticle
hub:publisher-id
aa41556-21
dcterms:dateCopyrighted
2022-01-01
dcterms:rights
© Euclid Collaboration 2022
dcterms:rightsHolder
Euclid Collaboration
hub:isPartOfThisJournal
n66:w