CERN Accelerating science

002862847 001__ 2862847
002862847 005__ 20241212044334.0
002862847 0248_ $$aoai:cds.cern.ch:2862847$$pcerncds:FULLTEXT$$pcerncds:CERN:FULLTEXT$$pcerncds:CERN
002862847 0247_ $$2DOI$$9arXiv$$a10.1051/0004-6361/202347526$$qpublication
002862847 037__ $$9arXiv$$aarXiv:2306.12368$$castro-ph.CO
002862847 035__ $$9arXiv$$aoai:arXiv.org:2306.12368
002862847 035__ $$9Inspire$$aoai:inspirehep.net:2670531$$d2024-12-11T16:10:01Z$$h2024-12-12T03:00:24Z$$mmarcxml$$ttrue$$uhttps://inspirehep.net/api/oai2d
002862847 035__ $$9Inspire$$a2670531
002862847 041__ $$aeng
002862847 100__ $$aFrusciante, N.$$jORCID:[email protected]$$uNaples U.$$vDepartment of Physics “E. Pancini”, University Federico II, Via Cinthia 6, 80126 Napoli, Italy
002862847 245__ $$9arXiv$$aEuclid: Constraining linearly scale-independent modifications of gravity with the spectroscopic and photometric primary probes
002862847 269__ $$c2023-06-21
002862847 260__ $$c2024-10-01
002862847 260__ $$c2024-10
002862847 300__ $$a22 p
002862847 520__ $$9EDP Sciences$$aContext. The future Euclid space satellite mission will offer an invaluable opportunity to constrain modifications to Einstein’s general relativity at cosmic scales. In this paper, we focus on modified gravity models characterised, at linear scales, by a scale-independent growth of perturbations while featuring different testable types of derivative screening mechanisms at smaller non-linear scales.Aims. We considered three specific models, namely Jordan-Brans-Dicke, a scalar-tensor theory with a flat potential, the normal branch of Dvali-Gabadadze-Porrati (nDGP) gravity, a braneworld model in which our Universe is a four-dimensional brane embedded in a five-dimensional Minkowski space-time, and k-mouflage gravity, an extension of k-essence scenarios with a universal coupling of the scalar field to matter. In preparation for real data, we provide forecasts from spectroscopic and photometric primary probes by Euclid on the cosmological parameters and the additional parameters of the models, respectively, ωBD, Ωгc and ϵ2,0, which quantify the deviations from general relativity. This analysis will improve our knowledge of the cosmology of these modified gravity models.Methods. The forecast analysis employs the Fisher matrix method applied to weak lensing (WL); photometric galaxy clustering (GCph), spectroscopic galaxy clustering (GCsp) and the cross-correlation (XC) between GCph and WL. For the Euclid survey specifications, we define three scenarios that are characterised by different cuts in the maximum multipole and wave number, to assess the constraining power of non-linear scales. For each model we considered two fiducial values for the corresponding model parameter.Results. In an optimistic setting at 68.3% confidence interval, we find the following percentage relative errors with Euclid alone: for log10 ωBD, with a fiducial value of ωBD = 800, 27.1% using GCsp alone, 3.6% using GCph+WL+XC and 3.2% using GCph+WL+XC+GCsp; for log10 Ωгc, with a fiducial value of Ωгc = 0.25, we find 93.4, 20 and 15% respectively; and finally, for ϵ2,0 = −0.04, we find 3.4%, 0.15%, and 0.14%. From the relative errors for fiducial values closer to their ΛCDM limits, we find that most of the constraining power is lost. Our results highlight the importance of the constraining power from non-linear scales.Key words: cosmology: theory / large-scale structure of Universe★ This paper is published on behalf of the Euclid Consortium.
002862847 520__ $$9arXiv$$aThe future Euclid space satellite mission will offer an invaluable opportunity to constrain modifications to Einstein's general relativity at cosmic scales. We focus on modified gravity models characterised, at linear scales, by a scale-independent growth of perturbations while featuring different testable types of derivative screening mechanisms at smaller non-linear scales. We considered three specific models, namely JBD, a scalar-tensor theory with a flat potential, the nDGP gravity, a braneworld model in which our Universe is a four-dimensional brane embedded in a five-dimensional Minkowski space-time, and $k$-mouflage (KM) gravity, an extension of $k$-essence scenarios with a universal coupling of the scalar field to matter. In preparation for real data, we provide forecasts from spectroscopic and photometric primary probes by Euclid on the cosmological parameters and the additional parameters of the models, respectively, $\omega_{\rm BD}$, $\Omega_{\rm rc}$ and $\epsilon_{2,0}$. The forecast analysis employs the Fisher matrix method applied to weak lensing (WL); photometric galaxy clustering (GCph), spectroscopic galaxy clustering (GCsp) and the cross-correlation (XC) between GCph and WL. In an optimistic setting at 68.3% confidence interval, we find the following percentage relative errors with Euclid alone: for $\log_{10}{\omega_{\rm BD}}$, with a fiducial value of $\omega_{\rm BD}=800$, 27.1% using GCsp alone, 3.6% using GCph+WL+XC and 3.2% using GCph+WL+XC+GCsp; for $\log_{10}{\Omega_{\rm rc}}$, with a fiducial value of $\Omega_{\rm rc}=0.25$, we find 93.4%, 20% and 15% respectively; and finally, for $\epsilon_{2,0}=-0.04$, we find 3.4%, 0.15%, and 0.14%. (abridged)
002862847 540__ $$3preprint$$aCC BY 4.0$$uhttp://creativecommons.org/licenses/by/4.0/
002862847 540__ $$3publication$$aCC BY 4.0$$uhttp://creativecommons.org/licenses/by/4.0/
002862847 542__ $$3publication$$dThe Authors$$g2024
002862847 595_D $$aV$$d2023-06-23$$sabs
002862847 65017 $$2arXiv$$agr-qc
002862847 65017 $$2SzGeCERN$$aGeneral Relativity and Cosmology
002862847 65017 $$2arXiv$$aastro-ph.CO
002862847 65017 $$2SzGeCERN$$aAstrophysics and Astronomy
002862847 693__ $$aEUCLID
002862847 690C_ $$aCERN
002862847 690C_ $$aARTICLE
002862847 700__ $$aPace, F.$$jORCID:0000-0001-8039-0480$$uTurin U.$$uINFN, Turin$$uTurin Observ.$$vDipartimento di Fisica, Università degli Studi di Torino, Via P. Giuria 1, 10125 Torino, Italy$$vINFN-Sezione di Torino, Via P. Giuria 1, 10125 Torino, Italy$$vINAF-Osservatorio Astrofisico di Torino, Via Osservatorio 20, 10025 Pino Torinese (TO), Italy
002862847 700__ $$aCardone, V.F.$$uRome Observ.$$uRome U.$$vINAF-Osservatorio Astronomico di Roma, Via Frascati 33, 00078 Monteporzio Catone, Italy$$vINFN-Sezione di Roma, Piazzale Aldo Moro, 2 - c/o Dipartimento di Fisica, Edificio G. Marconi, 00185 Roma, Italy
002862847 700__ $$aCasas, S.$$jORCID:0000-0002-4751-5138$$uUnlisted, GE$$vInstitute for Theoretical Particle Physics and Cosmology (TTK), RWTH Aachen University, 52056 Aachen, Germany
002862847 700__ $$aTutusaus, I.$$jORCID:0000-0002-3199-0399$$uGeneva U.$$uBarcelona, IEEC$$uIRAP, Toulouse$$vUniversité de Genève, Département de Physique Théorique and Centre for Astroparticle Physics, 24 quai Ernest-Ansermet, 1211 Genève 4, Switzerland$$vInstitute of Space Sciences (ICE, CSIC), Campus UAB, Carrer de Can Magrans, s/n, 08193 Barcelona, Spain$$vInstitut d’Estudis Espacials de Catalunya (IEEC), Carrer Gran Capitá 2-4, 08034 Barcelona, Spain$$vInstitut de Recherche en Astrophysique et Planétologie (IRAP), Université de Toulouse, CNRS, UPS, CNES, 14 Av. Edouard Belin, 31400 Toulouse, France
002862847 700__ $$aBallardini, M.$$jORCID:0000-0003-4481-3559$$uFerrara U.$$uBologna U.$$uBologna Observ.$$uINFN, Bologna$$vDipartimento di Fisica e Scienze della Terra, Universitá degli Studi di Ferrara, Via Giuseppe Saragat 1, 44122 Ferrara, Italy$$vDipartimento di Fisica e Astronomia, Universitá di Bologna, Via Gobetti 93/2, 40129 Bologna, Italy$$vINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy$$vINFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy
002862847 700__ $$aBellini, E.$$uINFN, Trieste$$uSISSA, Trieste$$uIFPU, Trieste$$uGeneva U.$$vINFN, Sezione di Trieste, Via Valerio 2, 34127 Trieste TS, Italy$$vIFPU, Institute for Fundamental Physics of the Universe, via Beirut 2, 34151 Trieste, Italy$$vSISSA, International School for Advanced Studies, Via Bonomea 265, 34136 Trieste TS, Italy$$vUniversité de Genève, Département de Physique Théorique and Centre for Astroparticle Physics, 24 quai Ernest-Ansermet, 1211 Genève 4, Switzerland
002862847 700__ $$aBenevento, G.$$jORCID:0000-0002-6999-2429$$uJohns Hopkins U.$$vJohns Hopkins University 3400 North Charles Street Baltimore, MD 21218, USA
002862847 700__ $$aBose, B.$$jORCID:0000-0003-1965-8614$$uEdinburgh U., Inst. Astron.$$uGeneva U.$$uZurich U.$$vInstitute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, UK$$vUniversité de Genève, Département de Physique Théorique and Centre for Astroparticle Physics, 24 quai Ernest-Ansermet, 1211 Genève 4, Switzerland$$vInstitute for Computational Science, University of Zurich, Winterthurerstrasse 190, 8057 Zurich, Switzerland
002862847 700__ $$aValageas, P.$$jORCID:0000-0002-5540-3320$$uIPhT, Saclay$$vInstitut de Physique Théorique, CEA, CNRS, Université Paris-Saclay 91191 Gif-sur-Yvette Cedex, France
002862847 700__ $$aBartolo, N.$$uU. Padua, Dept. Phys. Astron.$$uINFN, Padua$$uPadua Observ.$$vDipartimento di Fisica e Astronomia “G.Galilei”, Università di Padova, Via Marzolo 8, 35131 Padova, Italy$$vINFN-Padova, Via Marzolo 8, 35131 Padova, Italy$$vINAF-Osservatorio Astronomico di Padova, Via dell’Osservatorio 5, 35122 Padova, Italy
002862847 700__ $$aBrax, P.$$uIPhT, Saclay$$uCERN$$vInstitut de Physique Théorique, CEA, CNRS, Université Paris-Saclay 91191 Gif-sur-Yvette Cedex, France$$vCERN, Theoretical Physics Department, Geneva, Switzerland
002862847 700__ $$aFerreira, P.G.$$uOxford U.$$vDepartment of Physics, Oxford University, Keble Road, Oxford OX1 3RH, UK
002862847 700__ $$aFinelli, F.$$uBologna Observ.$$uINFN, Bologna$$vINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy$$vINFN-Bologna, Via Irnerio 46, 40126 Bologna, Italy
002862847 700__ $$aKoyama, K.$$jORCID:0000-0001-6727-6915$$uPortsmouth U., ICG$$vInstitute of Cosmology and Gravitation, University of Portsmouth, Portsmouth PO1 3FX, UK
002862847 700__ $$aLegrand, L.$$jORCID:0000-0003-0610-5252$$uGeneva U.$$vUniversité de Genève, Département de Physique Théorique and Centre for Astroparticle Physics, 24 quai Ernest-Ansermet, 1211 Genève 4, Switzerland
002862847 700__ $$aLombriser, L.$$jORCID:0000-0002-4681-9500$$uGeneva U.$$vUniversité de Genève, Département de Physique Théorique and Centre for Astroparticle Physics, 24 quai Ernest-Ansermet, 1211 Genève 4, Switzerland
002862847 700__ $$aPaoletti, D.$$jORCID:0000-0003-4761-6147$$uBologna Observ.$$uINFN, Bologna$$vINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy$$vINFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy
002862847 700__ $$aPietroni, M.$$jORCID:0000-0001-5480-5996$$uICJ, Lyon$$uParma U.$$vDipartimento di Scienze Matematiche, Fisiche e Informatiche, Università di Parma, Viale delle Scienze 7/A 43124 Parma, Italy$$vINFN Gruppo Collegato di Parma, Viale delle Scienze 7/A 43124 Parma, Italy
002862847 700__ $$aRozas-Fernández, A.$$jORCID:0000-0002-6131-2804$$uLisbon U.$$vInstituto de Astrofísica e Ciências do Espaço, Faculdade de Ciên-cias, Universidade de Lisboa, Campo Grande, 1749-016 Lisboa, Portugal
002862847 700__ $$aSakr, Z.$$jORCID:0000-0002-4823-3757$$uParis, Inst. Astrophys.$$uU. Heidelberg, ITP$$uUSJ, Beirut$$vInstitut d’Astrophysique de Paris, UMR 7095, CNRS, and Sorbonne Université, 98 bis boulevard Arago, 75014 Paris, France$$vInstitut für Theoretische Physik, University of Heidelberg, Philosophenweg 16, 69120 Heidelberg, Germany$$vUniversité St Joseph; Faculty of Sciences, Beirut, Lebanon
002862847 700__ $$aSilvestri, A.$$uLeiden U.$$vInstitute Lorentz, Leiden University, PO Box 9506, Leiden 2300 RA, The Netherlands
002862847 700__ $$aVernizzi, F.$$jORCID:0000-0003-3426-2802$$uIPhT, Saclay$$vInstitut de Physique Théorique, CEA, CNRS, Université Paris-Saclay 91191 Gif-sur-Yvette Cedex, France
002862847 700__ $$aWinther, H.A.$$jORCID:0000-0002-6325-2710$$uInst. Theor. Astrophys., Oslo$$vInstitute of Theoretical Astrophysics, University of Oslo, PO Box 1029 Blindern, 0315 Oslo, Norway
002862847 700__ $$aAghanim, N.$$uOrsay, IAS$$vUniversité Paris-Saclay, CNRS, Institut d’astrophysique spatiale, 91405, Orsay, France
002862847 700__ $$aAmendola, L.$$uU. Heidelberg, ITP$$vInstitut für Theoretische Physik, University of Heidelberg, Philosophenweg 16, 69120 Heidelberg, Germany
002862847 700__ $$aAuricchio, N.$$jORCID:0000-0003-4444-8651$$uBologna Observ.$$vINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy
002862847 700__ $$aAzzollini, R.$$uMullard Space Sci. Lab.$$vMullard Space Science Laboratory, University College London, Holmbury St Mary, Dorking, Surrey RH5 6NT, UK
002862847 700__ $$aBaldi, M.$$jORCID:0000-0003-4145-1943$$uBologna U.$$uBologna Observ.$$uINFN, Bologna$$vDipartimento di Fisica e Astronomia, Universitá di Bologna, Via Gobetti 93/2, 40129 Bologna, Italy$$vINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy$$vINFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy
002862847 700__ $$aBonino, D.$$uTurin Observ.$$vINAF-Osservatorio Astrofisico di Torino, Via Osservatorio 20, 10025 Pino Torinese (TO), Italy
002862847 700__ $$aBranchini, E.$$jORCID:0000-0002-0808-6908$$uGenoa U.$$uINFN, Genoa$$uINFN, Rome3$$vDipartimento di Fisica, Università degli studi di Genova, and INFN-Sezione di Genova, via Dodecaneso 33, 16146 Genova, Italy$$vINFN-Sezione di Roma Tre, Via della Vasca Navale 84, 00146 Roma, Italy
002862847 700__ $$aBrescia, M.$$jORCID:0000-0001-9506-5680$$uNaples U.$$uCapodimonte Observ.$$vDepartment of Physics “E. Pancini”, University Federico II, Via Cinthia 6, 80126 Napoli, Italy$$vINAF-Osservatorio Astronomico di Capodimonte, Via Moiariello 16, 80131 Napoli, Italy
002862847 700__ $$aBrinchmann, J.$$jORCID:0000-0003-4359-8797$$uPorto U., Astron. Dept.$$vInstituto de Astrofísica e Ciências do Espaço, Universidade do Porto, CAUP, Rua das Estrelas, PT4150-762 Porto, Portugal
002862847 700__ $$aCamera, S.$$jORCID:0000-0003-3399-3574$$uTurin U.$$uINFN, Turin$$uTurin Observ.$$vDipartimento di Fisica, Università degli Studi di Torino, Via P. Giuria 1, 10125 Torino, Italy$$vINFN-Sezione di Torino, Via P. Giuria 1, 10125 Torino, Italy$$vINAF-Osservatorio Astrofisico di Torino, Via Osservatorio 20, 10025 Pino Torinese (TO), Italy
002862847 700__ $$aCapobianco, V.$$jORCID:0000-0002-3309-7692$$uTurin Observ.$$vINAF-Osservatorio Astrofisico di Torino, Via Osservatorio 20, 10025 Pino Torinese (TO), Italy
002862847 700__ $$aCarbone, C.$$uIASF, Milan$$vINAF-IASF Milano, Via Alfonso Corti 12, 20133 Milano, Italy
002862847 700__ $$aCarretero, J.$$jORCID:0000-0002-3130-0204$$uBarcelona, IFAE$$vInstitut de Física d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology, Campus UAB, 08193 Bellaterra (Barcelona), Spain$$vPort d’Informació Científica, Campus UAB, C. Albareda s/n, 08193 Bellaterra (Barcelona), Spain
002862847 700__ $$aCastellano, M.$$jORCID:0000-0001-9875-8263$$uRome Observ.$$vINAF-Osservatorio Astronomico di Roma, Via Frascati 33, 00078 Monteporzio Catone, Italy
002862847 700__ $$aCavuoti, S.$$jORCID:0000-0002-3787-4196$$uCapodimonte Observ.$$uINFN, Naples$$vINAF-Osservatorio Astronomico di Capodimonte, Via Moiariello 16, 80131 Napoli, Italy$$vINFN section of Naples, Via Cinthia 6, 80126, Napoli, Italy
002862847 700__ $$aCimatti, A.$$uBologna U.$$uTrieste Observ.$$vDipartimento di Fisica e Astronomia “Augusto Righi” - Alma Mater Studiorum Università di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy$$vINAF-Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, 50125 Firenze, Italy
002862847 700__ $$aCledassou, R.$$jORCID:0000-0002-8313-2230$$uCNES, Toulouse$$uParis, IN2P3$$vCentre National d’Etudes Spatiales, Toulouse, France$$vInstitut national de physique nucléaire et de physique des particules, 3 rue Michel-Ange, 75794 Paris Cédex 16, France
002862847 700__ $$aCongedo, G.$$jORCID:0000-0003-2508-0046$$uEdinburgh U., Inst. Astron.$$vInstitute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, UK
002862847 700__ $$aConversi, L.$$jORCID:0000-0002-6710-8476$$uEuropean Space Agency$$uESA, Madrid$$vEuropean Space Agency/ESRIN, Largo Galileo Galilei 1, 00044 Frascati, Roma, Italy$$vESAC/ESA, Camino Bajo del Castillo, s/n., Urb. Villafranca del Castillo, 28692 Villanueva de la Cañada, Madrid, Spain
002862847 700__ $$aCopin, Y.$$jORCID:0000-0002-5317-7518$$uIP2I, Lyon$$vUniv Lyon, Univ Claude Bernard Lyon 1, CNRS/IN2P3, IP2I Lyon, UMR 5822, 69622 Villeurbanne, France
002862847 700__ $$aCorcione, L.$$jORCID:0000-0002-6497-5881$$uTurin Observ.$$vINAF-Osservatorio Astrofisico di Torino, Via Osservatorio 20, 10025 Pino Torinese (TO), Italy
002862847 700__ $$aCourbin, F.$$jORCID:0000-0003-0758-6510$$uLASTRO Observ.$$vInstitute of Physics, Laboratory of Astrophysics, Ecole Polytech-nique Fédérale de Lausanne (EPFL), Observatoire de Sauverny, 1290 Versoix, Switzerland
002862847 700__ $$aCropper, M.$$uMullard Space Sci. Lab.$$vMullard Space Science Laboratory, University College London, Holmbury St Mary, Dorking, Surrey RH5 6NT, UK
002862847 700__ $$aDa Silva, A.$$jORCID:0000-0002-6385-1609$$uLisbon U.$$vDepartamento de Física, Faculdade de Ciências, Universidade de Lisboa, Edifício C8, Campo Grande, PT1749-016 Lisboa, Portugal$$vInstituto de Astrofísica e Ciências do Espaço, Faculdade de Ciên-cias, Universidade de Lisboa, Campo Grande, 1749-016 Lisboa, Portugal
002862847 700__ $$aDegaudenzi, H.$$jORCID:0000-0002-5887-6799$$uU. Geneva (main)$$vDepartment of Astronomy, University of Geneva, ch. d’Ecogia 16, 1290 Versoix, Switzerland
002862847 700__ $$aDinis, J.$$uLisbon U.$$vInstituto de Astrofísica e Ciências do Espaço, Faculdade de Ciên-cias, Universidade de Lisboa, Campo Grande, 1749-016 Lisboa, Portugal$$vDepartamento de Física, Faculdade de Ciências, Universidade de Lisboa, Edifício C8, Campo Grande, PT1749-016 Lisboa, Portugal
002862847 700__ $$aDubath, F.$$uU. Geneva (main)$$vDepartment of Astronomy, University of Geneva, ch. d’Ecogia 16, 1290 Versoix, Switzerland
002862847 700__ $$aDupac, X.$$uESA, Madrid$$vESAC/ESA, Camino Bajo del Castillo, s/n., Urb. Villafranca del Castillo, 28692 Villanueva de la Cañada, Madrid, Spain
002862847 700__ $$aDusini, S.$$jORCID:0000-0002-1128-0664$$uINFN, Padua$$vINFN-Padova, Via Marzolo 8, 35131 Padova, Italy
002862847 700__ $$aFarrens, S.$$jORCID:0000-0002-9594-9387$$uAIM, Saclay$$vUniversité Paris-Saclay, Université Paris Cité, CEA, CNRS, Astro-physique, Instrumentation et Modélisation Paris-Saclay, 91191 Gif-sur-Yvette, France
002862847 700__ $$aFerriol, S.$$uIP2I, Lyon$$vUniv Lyon, Univ Claude Bernard Lyon 1, CNRS/IN2P3, IP2I Lyon, UMR 5822, 69622 Villeurbanne, France
002862847 700__ $$aFosalba, P.$$jORCID:0000-0002-1510-5214$$uBarcelona, IEEC$$vInstitut d’Estudis Espacials de Catalunya (IEEC), Carrer Gran Capitá 2-4, 08034 Barcelona, Spain$$vInstitute of Space Sciences (ICE, CSIC), Campus UAB, Carrer de Can Magrans, s/n, 08193 Barcelona, Spain
002862847 700__ $$aFrailis, M.$$jORCID:0000-0002-7400-2135$$uTrieste Observ.$$vINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy
002862847 700__ $$aFranceschi, E.$$jORCID:0000-0002-0585-6591$$uBologna Observ.$$vINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy
002862847 700__ $$aGaleotta, S.$$jORCID:0000-0002-3748-5115$$uTrieste Observ.$$vINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy
002862847 700__ $$aGillis, B.$$jORCID:0000-0002-4478-1270$$uEdinburgh U., Inst. Astron.$$vInstitute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, UK
002862847 700__ $$aGiocoli, C.$$jORCID:0000-0002-9590-7961$$uBologna Observ.$$uINFN, Bologna$$vINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy$$vIstituto Nazionale di Fisica Nucleare, Sezione di Bologna, Via Irnerio 46, 40126 Bologna, Italy
002862847 700__ $$aGrazian, A.$$jORCID:0000-0002-5688-0663$$uPadua Observ.$$vINAF-Osservatorio Astronomico di Padova, Via dell’Osservatorio 5, 35122 Padova, Italy
002862847 700__ $$aGrupp, F.$$uGarching, Max Planck Inst., MPE$$uMunich U.$$vMax Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, 85748 Garching, Germany$$vUniversitäts-Sternwarte München, Fakultät für Physik, Ludwig-Maximilians-Universität München, Scheinerstrasse 1, 81679 München, Germany
002862847 700__ $$aGuzzo, L.$$uMilan U.$$uINFN, Milan$$uBrera Observ.$$vDipartimento di Fisica “Aldo Pontremoli”, Università degli Studi di Milano, Via Celoria 16, 20133 Milano, Italy$$vINFN-Sezione di Milano, Via Celoria 16, 20133 Milano, Italy$$vINAF-Osservatorio Astronomico di Brera, Via Brera 28, 20122 Milano, Italy
002862847 700__ $$aHaugan, S.V. H.$$jORCID:0000-0001-9648-7260$$uInst. Theor. Astrophys., Oslo$$vInstitute of Theoretical Astrophysics, University of Oslo, PO Box 1029 Blindern, 0315 Oslo, Norway
002862847 700__ $$aHolmes, W.$$uCaltech, JPL$$vJet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA, 91109, USA
002862847 700__ $$aHormuth, F.$$uUnlisted, DE$$vvon Hoerner & Sulger GmbH, SchloßPlatz 8, 68723 Schwetzingen, Germany
002862847 700__ $$aHornstrup, A.$$jORCID:0000-0002-3363-0936$$uDenmark, Tech. U.$$vTechnical University of Denmark, Elektrovej 327, 2800 Kgs. Lyngby, Denmark
002862847 700__ $$aJahnke, K.$$jORCID:0000-0003-3804-2137$$uHeidelberg, Max Planck Inst. Astron.$$vMax-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany
002862847 700__ $$aKermiche, S.$$jORCID:0000-0002-0302-5735$$uMarseille, CPPM$$vAix-Marseille Université, CNRS/IN2P3, CPPM, Marseille, France
002862847 700__ $$aKiessling, A.$$jORCID:0000-0002-2590-1273$$uCaltech, JPL$$vJet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA, 91109, USA
002862847 700__ $$aKilbinger, M.$$uAIM, Saclay$$vUniversité Paris-Saclay, Université Paris Cité, CEA, CNRS, Astro-physique, Instrumentation et Modélisation Paris-Saclay, 91191 Gif-sur-Yvette, France
002862847 700__ $$aKitching, T.$$jORCID:0000-0002-4061-4598$$uMullard Space Sci. Lab.$$vMullard Space Science Laboratory, University College London, Holmbury St Mary, Dorking, Surrey RH5 6NT, UK
002862847 700__ $$aKunz, M.$$jORCID:0000-0002-3052-7394$$uGeneva U.$$vUniversité de Genève, Département de Physique Théorique and Centre for Astroparticle Physics, 24 quai Ernest-Ansermet, 1211 Genève 4, Switzerland
002862847 700__ $$aKurki-Suonio, H.$$jORCID:0000-0002-4618-3063$$uHelsinki Inst. of Phys.$$vDepartment of Physics and Helsinki Institute of Physics, Gustaf Hällströmin katu 2, 00014 University of Helsinki, Finland
002862847 700__ $$aLigori, S.$$jORCID:0000-0003-4172-4606$$uTurin Observ.$$vINAF-Osservatorio Astrofisico di Torino, Via Osservatorio 20, 10025 Pino Torinese (TO), Italy
002862847 700__ $$aLilje, P.B.$$jORCID:0000-0003-4324-7794$$uInst. Theor. Astrophys., Oslo$$vInstitute of Theoretical Astrophysics, University of Oslo, PO Box 1029 Blindern, 0315 Oslo, Norway
002862847 700__ $$aLloro, I.$$uASTRON, Dwingeloo$$vNOVA optical infrared instrumentation group at ASTRON, Oude Hoogeveensedijk 4, 7991PD Dwingeloo, The Netherlands
002862847 700__ $$aMaiorano, E.$$jORCID:0000-0003-2593-4355$$uBologna Observ.$$vINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy
002862847 700__ $$aMansutti, O.$$jORCID:0000-0001-5758-4658$$uTrieste Observ.$$vINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy
002862847 700__ $$aMarggraf, O.$$jORCID:0000-0001-7242-3852$$uArgelander Inst. Astron.$$vArgelander-Institut für Astronomie, Universität Bonn, Auf dem Hügel 71, 53121 Bonn, Germany
002862847 700__ $$aMarkovic, K.$$jORCID:0000-0001-6764-073X$$uCaltech, JPL$$vJet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA, 91109, USA
002862847 700__ $$aMarulli, F.$$jORCID:0000-0002-8850-0303$$uU. Bologna, DIFA$$uBologna Observ.$$uINFN, Bologna$$vDipartimento di Fisica e Astronomia “Augusto Righi” - Alma Mater Studiorum Università di Bologna, via Piero Gobetti 93/2, 40129 Bologna, Italy$$vINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy$$vINFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy
002862847 700__ $$aMassey, R.$$jORCID:0000-0002-6085-3780$$uDurham U., ICC$$vDepartment of Physics, Institute for Computational Cosmology, Durham University, South Road, DH1 3LE, UK
002862847 700__ $$aMedinaceli, E.$$jORCID:0000-0002-4040-7783$$uBologna Observ.$$vINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy
002862847 700__ $$aMeneghetti, M.$$jORCID:0000-0003-1225-7084$$uINFN, Bologna$$uBologna Observ.$$vINFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy$$vINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy
002862847 700__ $$aMeylan, G.$$uLASTRO Observ.$$vInstitute of Physics, Laboratory of Astrophysics, Ecole Polytech-nique Fédérale de Lausanne (EPFL), Observatoire de Sauverny, 1290 Versoix, Switzerland
002862847 700__ $$aMoresco, M.$$jORCID:0000-0002-7616-7136$$uU. Bologna, DIFA$$uBologna Observ.$$vDipartimento di Fisica e Astronomia “Augusto Righi” - Alma Mater Studiorum Università di Bologna, via Piero Gobetti 93/2, 40129 Bologna, Italy$$vINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy
002862847 700__ $$aMoscardini, L.$$jORCID:0000-0002-3473-6716$$uU. Bologna, DIFA$$uBologna Observ.$$uINFN, Bologna$$vDipartimento di Fisica e Astronomia “Augusto Righi” - Alma Mater Studiorum Università di Bologna, via Piero Gobetti 93/2, 40129 Bologna, Italy$$vINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy$$vINFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy
002862847 700__ $$aMunari, E.$$jORCID:0000-0002-1751-5946$$uTrieste Observ.$$vINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy
002862847 700__ $$aNiemi, S.M.$$uESTEC, Noordwijk$$vEuropean Space Agency/ESTEC, Keplerlaan 1, 2201 AZ Noordwijk, The Netherlands
002862847 700__ $$aNightingale, J.$$jORCID:0000-0002-8987-7401$$uDurham U., ICC$$vDepartment of Physics, Institute for Computational Cosmology, Durham University, South Road, DH1 3LE, UK
002862847 700__ $$aPadilla, C.$$jORCID:0000-0001-7951-0166$$uBarcelona, IFAE$$vInstitut de Física d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology, Campus UAB, 08193 Bellaterra (Barcelona), Spain
002862847 700__ $$aPaltani, S.$$uU. Geneva (main)$$vDepartment of Astronomy, University of Geneva, ch. d’Ecogia 16, 1290 Versoix, Switzerland
002862847 700__ $$aPasian, F.$$uTrieste Observ.$$vINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy
002862847 700__ $$aPedersen, K.$$uAarhus U.$$vDepartment of Physics and Astronomy, University of Aarhus, Ny Munkegade 120, 8000 Aarhus C, Denmark
002862847 700__ $$aPercival, W.J.$$jORCID:0000-0002-0644-5727$$uWaterloo U., Math. Dept.$$uWaterloo U.$$uPerimeter Inst. Theor. Phys.$$vCentre for Astrophysics, University of Waterloo, Waterloo, Ontario N2L 3G1, Canada$$vDepartment of Physics and Astronomy, University of Waterloo, Waterloo, Ontario N2L 3G1, Canada$$vPerimeter Institute for Theoretical Physics, Waterloo, Ontario N2L 2Y5, Canada
002862847 700__ $$aPettorino, V.$$uAIM, Saclay$$vUniversité Paris-Saclay, Université Paris Cité, CEA, CNRS, Astro-physique, Instrumentation et Modélisation Paris-Saclay, 91191 Gif-sur-Yvette, France
002862847 700__ $$aPolenta, G.$$jORCID:0000-0003-4067-9196$$uASI, Rome$$vSpace Science Data Center, Italian Space Agency, via del Politecnico snc, 00133 Roma, Italy
002862847 700__ $$aPoncet, M.$$uCNES, Toulouse$$vCentre National d’Etudes Spatiales, Toulouse, France
002862847 700__ $$aPopa, L.$$uBucharest, Inst. Space Science$$vInstitute of Space Science, Bucharest, 077125, Romania
002862847 700__ $$aRaison, F.$$uGarching, Max Planck Inst., MPE$$vMax Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, 85748 Garching, Germany
002862847 700__ $$aRebolo, R.$$uIAC, La Laguna$$uLaguna U., Tenerife$$vInstituto de Astrofísica de Canarias, Calle Vía Láctea s/n, 38204, San Cristóbal de La Laguna, Tenerife, Spain$$vDepartamento de Astrofísica, Universidad de La Laguna, 38206, La Laguna, Tenerife, Spain
002862847 700__ $$aRenzi, A.$$jORCID:0000-0001-9856-1970$$uU. Padua, Dept. Phys. Astron.$$uINFN, Padua$$vDipartimento di Fisica e Astronomia “G.Galilei”, Università di Padova, Via Marzolo 8, 35131 Padova, Italy$$vINFN-Padova, Via Marzolo 8, 35131 Padova, Italy
002862847 700__ $$aRhodes, J.$$uCaltech, JPL$$vJet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA, 91109, USA
002862847 700__ $$aRiccio, G.$$uCapodimonte Observ.$$vINAF-Osservatorio Astronomico di Capodimonte, Via Moiariello 16, 80131 Napoli, Italy
002862847 700__ $$aRomelli, E.$$jORCID:0000-0003-3069-9222$$uTrieste Observ.$$vINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy
002862847 700__ $$aSaglia, R.$$jORCID:0000-0003-0378-7032$$uGarching, Max Planck Inst., MPE$$uMunich U.$$vMax Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, 85748 Garching, Germany$$vUniversitäts-Sternwarte München, Fakultät für Physik, Ludwig-Maximilians-Universität München, Scheinerstrasse 1, 81679 München, Germany
002862847 700__ $$aSapone, D.$$jORCID:0000-0001-7089-4503$$uChile U., Beauchef$$vDepartamento de Física, FCFM, Universidad de Chile, Blanco Encalada 2008, Santiago, Chile
002862847 700__ $$aSartoris, B.$$uMunich U.$$uTrieste Observ.$$vUniversitäts-Sternwarte München, Fakultät für Physik, Ludwig-Maximilians-Universität München, Scheinerstrasse 1, 81679 München, Germany
002862847 700__ $$aSecroun, A.$$jORCID:0000-0003-0505-3710$$uMarseille, CPPM$$vAix-Marseille Université, CNRS/IN2P3, CPPM, Marseille, France
002862847 700__ $$aSeidel, G.$$jORCID:0000-0003-2907-353X$$uHeidelberg, Max Planck Inst. Astron.$$vMax-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany
002862847 700__ $$aSirignano, C.$$jORCID:0000-0002-0995-7146$$uU. Padua, Dept. Phys. Astron.$$uINFN, Padua$$vDipartimento di Fisica e Astronomia “G.Galilei”, Università di Padova, Via Marzolo 8, 35131 Padova, Italy$$vINFN-Padova, Via Marzolo 8, 35131 Padova, Italy
002862847 700__ $$aSirri, G.$$jORCID:0000-0003-2626-2853$$uINFN, Bologna$$vINFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy
002862847 700__ $$aStanco, L.$$jORCID:0000-0002-9706-5104$$uINFN, Padua$$vINFN-Padova, Via Marzolo 8, 35131 Padova, Italy
002862847 700__ $$aSurace, C.$$jORCID:0000-0003-2592-0113$$uMarseille, Lab. Astrophys.$$vAix-Marseille Université, CNRS, CNES, LAM, Marseille, France
002862847 700__ $$aTallada-Crespí, P.$$uMadrid, CIEMAT$$uMadrid, Escuela Tec. Sup. Ing. Ind.$$uBarcelona, IFAE$$vCentro de Investigaciones Energéticas, Medioambientales y Tec-nológicas (CIEMAT), Avenida Complutense 40, 28040 Madrid, Spain$$vPort d’Informació Científica, Campus UAB, C. Albareda s/n, 08193 Bellaterra (Barcelona), Spain
002862847 700__ $$aTaylor, A.N.$$uEdinburgh U., Inst. Astron.$$vInstitute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, UK
002862847 700__ $$aTereno, I.$$uLisbon U.$$uLisbon Astron. Observ.$$vDepartamento de Física, Faculdade de Ciências, Universidade de Lisboa, Edifício C8, Campo Grande, PT1749-016 Lisboa, Portugal$$vInstituto de Astrofísica e Ciências do Espaço, Faculdade de Ciên-cias, Universidade de Lisboa, Tapada da Ajuda, 1349-018 Lisboa, Portugal
002862847 700__ $$aToledo-Moreo, R.$$jORCID:0000-0002-2997-4859$$uCartagena Politecnica U.$$vUniversidad Politécnica de Cartagena, Departamento de Electrónica y Tecnología de Computadoras, 30202 Cartagena, Spain
002862847 700__ $$aTorradeflot, F.$$jORCID:0000-0003-1160-1517$$uMadrid, CIEMAT$$uMadrid, Escuela Tec. Sup. Ing. Ind.$$uBarcelona, IFAE$$vCentro de Investigaciones Energéticas, Medioambientales y Tec-nológicas (CIEMAT), Avenida Complutense 40, 28040 Madrid, Spain$$vPort d’Informació Científica, Campus UAB, C. Albareda s/n, 08193 Bellaterra (Barcelona), Spain
002862847 700__ $$aValentijn, E.A.$$uKapteyn Astron. Inst., Groningen$$vKapteyn Astronomical Institute, University of Groningen, PO Box 800, 9700 AV Groningen, The Netherlands
002862847 700__ $$aValenziano, L.$$jORCID:0000-0002-1170-0104$$uBologna Observ.$$uINFN, Bologna$$vINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy$$vINFN-Bologna, Via Irnerio 46, 40126 Bologna, Italy
002862847 700__ $$aVassallo, T.$$jORCID:0000-0001-6512-6358$$uTrieste Observ.$$vINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy
002862847 700__ $$aKleijn, G.A. Verdoes$$uKapteyn Astron. Inst., Groningen$$vKapteyn Astronomical Institute, University of Groningen, PO Box 800, 9700 AV Groningen, The Netherlands
002862847 700__ $$aWang, Y.$$jORCID:0000-0002-4749-2984$$uCaltech$$vInfrared Processing and Analysis Center, California Institute of Technology, Pasadena, CA 91125, USA
002862847 700__ $$aZacchei, A.$$jORCID:0000-0003-0396-1192$$uTrieste Observ.$$vINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy
002862847 700__ $$aZamorani, G.$$jORCID:0000-0002-2318-301X$$uBologna Observ.$$vINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy
002862847 700__ $$aZoubian, J.$$uMarseille, CPPM$$vAix-Marseille Université, CNRS/IN2P3, CPPM, Marseille, France
002862847 700__ $$aScottez, V.$$uParis, Inst. Astrophys.$$vInstitut d’Astrophysique de Paris, 98bis Boulevard Arago, 75014 Paris, France
002862847 710__ $$gEuclid Collaboration
002862847 773__ $$cA133$$mpublication$$pAstron. Astrophys.$$v690$$xA&A 690, A133 (2024)$$y2024
002862847 8564_ $$82460171$$s129988$$uhttp://cds.cern.ch/record/2862847/files/JBD1_Pes.png$$y00010 68.3\% and 95.4\%  joint marginal error contours on the cosmological parameters for JBD1 (left panel) and JBD2 (right panel) in the pessimistic case. In red \GCsp, in blue  WL+XC+\GCph\ and in green \GCsp+WL+XC+\GCph.
002862847 8564_ $$82460172$$s10887$$uhttp://cds.cern.ch/record/2862847/files/barplot_scales_all.png$$y00003 Marginalised $1\sigma$ errors on the models' parameters relative to their corresponding fiducial values, for JBD (case 1 in blue and case 2 in cyan), nDGP (case 1 in green and case 2 in light green) and KM (case 1 in red and case 2 in light red). We show the marginalised $1\sigma$ errors for \GCsp\ in the optimistic (dotted area), pessimistic (dashed area) and quasi-linear (filled area) scenarios (top panel), for WL+XC+\GCph\ in the optimistic and pessimistic cases (central panel) and for the \GCsp+WL+XC+\GCph\ in the the optimistic and pessimistic cases.
002862847 8564_ $$82460173$$s103265$$uhttp://cds.cern.ch/record/2862847/files/nDGP1_Opt.png$$y00006 68.3\% and 95.4\% joint marginal error contours on the cosmological parameters for nDGP1 (left panel) and nDGP2 (right panel) in the optimistic case. In red \GCsp, in blue  WL+XC+\GCph\ and in green \GCsp+WL+XC+\GCph.
002862847 8564_ $$82460174$$s93288$$uhttp://cds.cern.ch/record/2862847/files/nDGP2_Opt.png$$y00007 68.3\% and 95.4\% joint marginal error contours on the cosmological parameters for nDGP1 (left panel) and nDGP2 (right panel) in the optimistic case. In red \GCsp, in blue  WL+XC+\GCph\ and in green \GCsp+WL+XC+\GCph.
002862847 8564_ $$82460175$$s141932$$uhttp://cds.cern.ch/record/2862847/files/JBD2_Pes.png$$y00011 68.3\% and 95.4\%  joint marginal error contours on the cosmological parameters for JBD1 (left panel) and JBD2 (right panel) in the pessimistic case. In red \GCsp, in blue  WL+XC+\GCph\ and in green \GCsp+WL+XC+\GCph.
002862847 8564_ $$82460176$$s92095$$uhttp://cds.cern.ch/record/2862847/files/JBD2_Opt.png$$y00005 68.3\% and 95.4\% joint marginal error contours on the cosmological parameters for JBD1 (left panel) and JBD2 (right panel) in the optimistic case. In red \GCsp, in blue WL+XC+\GCph\ and in green \GCsp+WL+XC+\GCph.
002862847 8564_ $$82460177$$s6364$$uhttp://cds.cern.ch/record/2862847/files/barplot_scales_photo.png$$y00002 Marginalised $1\sigma$ errors on the model parameters relative to their corresponding fiducial values, for JBD (case 1 in blue and case 2 in cyan), nDGP (case 1 in green and case 2 in light green), and KM (case 1 in red and case 2 in light red). We show the marginalised $1\sigma$ errors for \GCsp\ in the optimistic (dotted area), pessimistic (dashed area) and quasi-linear (filled area) scenarios (top panel), for WL+XC+\GCph\ in the optimistic and pessimistic cases (central panel) and for the \GCsp+WL+XC+\GCph\ in the the optimistic and pessimistic cases.
002862847 8564_ $$82460178$$s123400$$uhttp://cds.cern.ch/record/2862847/files/KM1_Pes.png$$y00014 68.3\% and 95.4\%  joint marginal error contours on the cosmological parameters for KM1 (left panel) and KM2 (right panel) in the pessimistic case. In red \GCsp, in blue  WL+XC+\GCph\ and in green \GCsp+WL+XC+\GCph.
002862847 8564_ $$82460179$$s132482$$uhttp://cds.cern.ch/record/2862847/files/nDGP2_Pes.png$$y00013 68.3\% and 95.4\% joint marginal error contours on the cosmological parameters for nDGP1 (left panel) and nDGP2 (right panel) in the pessimistic case. In red \GCsp, in blue  WL+XC+\GCph\ and in green \GCsp+WL+XC+\GCph.
002862847 8564_ $$82460180$$s9557$$uhttp://cds.cern.ch/record/2862847/files/barplot_scales_spec.png$$y00001 Marginalised $1\sigma$ errors on the models' parameters relative to their corresponding fiducial values, for JBD (case 1 in blue and case 2 in cyan), nDGP (case 1 in green and case 2 in light green) and KM (case 1 in red and case 2 in light red). We show the marginalised $1\sigma$ errors for \GCsp\ in the optimistic (dotted area), pessimistic (dashed area) and quasi-linear (filled area) scenarios (top panel), for WL+XC+\GCph\ in the optimistic and pessimistic cases (central panel) and for the \GCsp+WL+XC+\GCph\ in the the optimistic and pessimistic cases.
002862847 8564_ $$82460181$$s6429926$$uhttp://cds.cern.ch/record/2862847/files/2306.12368.pdf$$yFulltext
002862847 8564_ $$82460182$$s132368$$uhttp://cds.cern.ch/record/2862847/files/nDGP1_Pes.png$$y00012 68.3\% and 95.4\% joint marginal error contours on the cosmological parameters for nDGP1 (left panel) and nDGP2 (right panel) in the pessimistic case. In red \GCsp, in blue  WL+XC+\GCph\ and in green \GCsp+WL+XC+\GCph.
002862847 8564_ $$82460183$$s139303$$uhttp://cds.cern.ch/record/2862847/files/KM2_Pes.png$$y00015 68.3\% and 95.4\%  joint marginal error contours on the cosmological parameters for KM1 (left panel) and KM2 (right panel) in the pessimistic case. In red \GCsp, in blue  WL+XC+\GCph\ and in green \GCsp+WL+XC+\GCph.
002862847 8564_ $$82460184$$s119981$$uhttp://cds.cern.ch/record/2862847/files/JBD1_Pes_AllZ.png$$y00016 68.3\% and 95.4\% joint marginal error contours on the cosmological parameters for JBD1 (left panel) and JBD2 (right panel) in the pessimistic case without the redshift cut at $z<0.9$ (see the text for details). In red \GCsp, in blue WL+XC+\GCph\ and in green \GCsp+WL+XC+\GCph.
002862847 8564_ $$82460185$$s114864$$uhttp://cds.cern.ch/record/2862847/files/JBD2_Pes_AllZ.png$$y00017 68.3\% and 95.4\% joint marginal error contours on the cosmological parameters for JBD1 (left panel) and JBD2 (right panel) in the pessimistic case without the redshift cut at $z<0.9$ (see the text for details). In red \GCsp, in blue WL+XC+\GCph\ and in green \GCsp+WL+XC+\GCph.
002862847 8564_ $$82460186$$s109621$$uhttp://cds.cern.ch/record/2862847/files/KM2_Opt.png$$y00009 68.3\% and 95.4\%  joint marginal error contours on the cosmological parameters for KM1 (left panel) and KM2 (right panel) in the optimistic case. In red \GCsp, in blue  WL+XC+\GCph\ and in green \GCsp+WL+XC+\GCph.
002862847 8564_ $$82460187$$s102440$$uhttp://cds.cern.ch/record/2862847/files/KM1_Opt.png$$y00008 68.3\% and 95.4\%  joint marginal error contours on the cosmological parameters for KM1 (left panel) and KM2 (right panel) in the optimistic case. In red \GCsp, in blue  WL+XC+\GCph\ and in green \GCsp+WL+XC+\GCph.
002862847 8564_ $$82460188$$s107788$$uhttp://cds.cern.ch/record/2862847/files/MGcomparison-CellsPk-3Models-new.png$$y00000 Large-scale structure observables for the different MG models considered in this work evaluated at the fiducial values of the model parameters used for the Fisher matrix analysis. {\bf Top Left}: The linear (dashed) and nonlinear (solid lines) matter power spectrum $P_{\delta \delta}(z,k)$ entering Eqs.~(\ref{eq:pk_dw}) and (\ref{eq:ISTrecipe}), respectively, evaluated at redshift $z=0$, for KM1 ($\epsilon_{2,0}=-0.04$, blue), JBD1 ($\omega_{\rm BD}=800$, red) and nDGP1 ($\Omega_{\rm rc}=0.25$, green). {\bf Top Right}: Ratio of the matter power spectra for the above mentioned models with respect to their \lcdm\ counterpart with the same value of $\sigma_8$ today, both for the linear (dashed) and nonlinear (solid) cases. While for nDGP1 and JBD1 the linear ratio remains constant, in the case of KM1 the ratio shows large-scale damping and oscillatory features that appear at scales around $k \approx 0.1\,h\, \mathrm{Mpc}^{-1}$. {\bf Bottom Left}: Cosmic shear (WL) angular power spectra for the first bin $i=j=1$, defined in Eq.~(\ref{eq:ISTrecipe}) for the three models considered above, with the same legend labels. {\bf Bottom Right}: Ratio of the cosmic shear $C_{i,j}(\ell)$ to their \lcdm\ counterpart, for the bin combination $i=j=1$. For JBD1 and nDGP1 the suppression in the nonlinear power spectrum can also be seen as a suppression of the lensing angular spectra. For KM1, however, although the nonlinear power spectrum is also decreased at small scales the lensing enhancement function $\Sigma$ defined in Eq.~(\ref{mu_Sigma_KM}) is larger than 1 at $z>0$, giving an overall increase in the lensing $C_{i,j}(\ell)$ when compared to \lcdm.
002862847 8564_ $$82460189$$s96933$$uhttp://cds.cern.ch/record/2862847/files/JBD1_Opt.png$$y00004 68.3\% and 95.4\% joint marginal error contours on the cosmological parameters for JBD1 (left panel) and JBD2 (right panel) in the optimistic case. In red \GCsp, in blue WL+XC+\GCph\ and in green \GCsp+WL+XC+\GCph.
002862847 8564_ $$82545051$$s127908$$uhttp://cds.cern.ch/record/2862847/files/KM1_Pes_hbug.png$$y00014 68.3\% and 95.4\%  joint marginal error contours on the cosmological parameters for KM1 (left panel) and KM2 (right panel) in the pessimistic case. In red, we plot \GCsp, in blue, we plot  WL+XC+\GCph\ and in green, we plot \GCsp+WL+XC+\GCph.
002862847 8564_ $$82545052$$s142265$$uhttp://cds.cern.ch/record/2862847/files/nDGP1_Pes_hbug.png$$y00012 68.3\% and 95.4\% joint marginal error contours on the cosmological parameters for nDGP1 (left panel) and nDGP2 (right panel) in the pessimistic case. In red, we plot \GCsp, in blue, we plot  WL+XC+\GCph\ and in green, we plot \GCsp+WL+XC+\GCph.
002862847 8564_ $$82545053$$s105835$$uhttp://cds.cern.ch/record/2862847/files/JBD1_Opt_hbug.png$$y00004 68.3\% and 95.4\% joint marginal error contours on the cosmological parameters for JBD1 (left panel) and JBD2 (right panel) in the optimistic case. In red, we plot \GCsp, in blue, we plot WL+XC+\GCph\ and in green we plot \GCsp+WL+XC+\GCph.
002862847 8564_ $$82545054$$s7891$$uhttp://cds.cern.ch/record/2862847/files/barplot_scales_all_hbug.png$$y00003 Marginalised $1\sigma$ errors on the model parameters relative to their corresponding fiducial values, for JBD (case 1 in blue and case 2 in cyan), nDGP (case 1 in green and case 2 in light green), and KM (case 1 in red and case 2 in light red). We show the marginalised $1\sigma$ errors for \GCsp\ in the optimistic (dotted area), pessimistic (dashed area) and quasi-linear (filled area) scenarios (top panel), for WL+XC+\GCph\ in the optimistic and pessimistic cases (central panel) and for the \GCsp+WL+XC+\GCph\ in the the optimistic and pessimistic cases.
002862847 8564_ $$82545055$$s108515$$uhttp://cds.cern.ch/record/2862847/files/KM1_Opt_hbug.png$$y00008 68.3\% and 95.4\% joint marginal error contours on the cosmological parameters for KM1 (left panel) and KM2 (right panel) in the optimistic case. In red, we plot \GCsp, in blue, we plot WL+XC+\GCph\ and in green, we plot \GCsp+WL+XC+\GCph.
002862847 8564_ $$82545056$$s101309$$uhttp://cds.cern.ch/record/2862847/files/JBD2_Opt_hbug.png$$y00005 68.3\% and 95.4\% joint marginal error contours on the cosmological parameters for JBD1 (left panel) and JBD2 (right panel) in the optimistic case. In red, we plot \GCsp, in blue, we plot WL+XC+\GCph\ and in green we plot \GCsp+WL+XC+\GCph.
002862847 8564_ $$82545057$$s6605$$uhttp://cds.cern.ch/record/2862847/files/barplot_scales_spec_hbug.png$$y00001 Marginalised $1\sigma$ errors on the model parameters relative to their corresponding fiducial values, for JBD (case 1 in blue and case 2 in cyan), nDGP (case 1 in green and case 2 in light green), and KM (case 1 in red and case 2 in light red). We show the marginalised $1\sigma$ errors for \GCsp\ in the optimistic (dotted area), pessimistic (dashed area) and quasi-linear (filled area) scenarios (top panel), for WL+XC+\GCph\ in the optimistic and pessimistic cases (central panel) and for the \GCsp+WL+XC+\GCph\ in the the optimistic and pessimistic cases.
002862847 8564_ $$82545058$$s101832$$uhttp://cds.cern.ch/record/2862847/files/nDGP2_Opt_hbug.png$$y00007 68.3\% and 95.4\% joint marginal error contours on the cosmological parameters for nDGP1 (left panel) and nDGP2 (right panel) in the optimistic case. In red, we plot \GCsp, in blue, we plot  WL+XC+\GCph\ and in green we plot \GCsp+WL+XC+\GCph.
002862847 8564_ $$82545059$$s121441$$uhttp://cds.cern.ch/record/2862847/files/KM2_Opt_hbug.png$$y00009 68.3\% and 95.4\% joint marginal error contours on the cosmological parameters for KM1 (left panel) and KM2 (right panel) in the optimistic case. In red, we plot \GCsp, in blue, we plot WL+XC+\GCph\ and in green, we plot \GCsp+WL+XC+\GCph.
002862847 8564_ $$82545060$$s117522$$uhttp://cds.cern.ch/record/2862847/files/AAnew-MGcomparison-CellsPk-3Models-new.png$$y00000 Large-scale structure observables for the different MG models evaluated at the fiducial values of the model parameters used for the Fisher matrix analysis. {\bf Top left}: Linear (dashed) and non-linear (solid lines) matter power spectrum $P_{\delta \delta}(z,k)$ entering Eqs.~(\ref{eq:pk_dw}) and (\ref{eq:ISTrecipe}), respectively, evaluated at redshift $z=0$, for KM1 ($\epsilon_{2,0}=-0.04$, blue), JBD1 ($\omega_{\rm BD}=800$, red) and nDGP1 ($\Omega_{\rm rc}=0.25$, green). {\bf Top right}: Ratio of the matter power spectra for the above mentioned models with respect to their \lcdm\ counterpart with the same value of $\sigma_8$ today, for the linear (dashed) and non-linear (solid) cases. {\bf Bottom left}: Cosmic shear (WL) angular power spectra for the auto-correlation of the first photometric bin $C^{\rm WL}_{1,1}(\ell)$ (solid line) and the cross-correlation of the first and last bin $C^{\rm WL}_{1,10}(\ell)$ (dotted line), defined in Eq.~(\ref{eq:ISTrecipe}) for the three models considered above, with the same colour labelling. {\bf Bottom right}: Ratio of the cosmic shear $C_{i,j}(\ell)$ to their \lcdm\ counterpart, for the bin combination $i=j=1$ and $i=1; j=10$.
002862847 8564_ $$82545061$$s141970$$uhttp://cds.cern.ch/record/2862847/files/nDGP2_Pes_hbug.png$$y00013 68.3\% and 95.4\% joint marginal error contours on the cosmological parameters for nDGP1 (left panel) and nDGP2 (right panel) in the pessimistic case. In red, we plot \GCsp, in blue, we plot  WL+XC+\GCph\ and in green, we plot \GCsp+WL+XC+\GCph.
002862847 8564_ $$82545062$$s145603$$uhttp://cds.cern.ch/record/2862847/files/JBD1_Pes_hbug.png$$y00010 68.3\% and 95.4\%  joint marginal error contours on the cosmological parameters for JBD1 (left panel) and JBD2 (right panel) in the pessimistic case. In red, we plot \GCsp, in blue, we plot  WL+XC+\GCph\ and in green, we plot \GCsp+WL+XC+\GCph.
002862847 8564_ $$82545063$$s153707$$uhttp://cds.cern.ch/record/2862847/files/KM2_Pes_hbug.png$$y00015 68.3\% and 95.4\%  joint marginal error contours on the cosmological parameters for KM1 (left panel) and KM2 (right panel) in the pessimistic case. In red, we plot \GCsp, in blue, we plot  WL+XC+\GCph\ and in green, we plot \GCsp+WL+XC+\GCph.
002862847 8564_ $$82545064$$s156766$$uhttp://cds.cern.ch/record/2862847/files/JBD2_Pes_hbug.png$$y00011 68.3\% and 95.4\%  joint marginal error contours on the cosmological parameters for JBD1 (left panel) and JBD2 (right panel) in the pessimistic case. In red, we plot \GCsp, in blue, we plot  WL+XC+\GCph\ and in green, we plot \GCsp+WL+XC+\GCph.
002862847 8564_ $$82545065$$s109535$$uhttp://cds.cern.ch/record/2862847/files/nDGP1_Opt_hbug.png$$y00006 68.3\% and 95.4\% joint marginal error contours on the cosmological parameters for nDGP1 (left panel) and nDGP2 (right panel) in the optimistic case. In red, we plot \GCsp, in blue, we plot  WL+XC+\GCph\ and in green we plot \GCsp+WL+XC+\GCph.
002862847 8564_ $$82626312$$s6854826$$uhttp://cds.cern.ch/record/2862847/files/Publication.pdf$$yFulltext
002862847 8564_ $$82690507$$s6854826$$uhttp://cds.cern.ch/record/2862847/files/document.pdf$$yFulltext
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