Euclid Preparation. Improving Cosmological Constraints Using a New Multi-Tracer Method with the Spectroscopic and Photometric Samples
F. Dournac,A. Blanchard,S. Ilic,B. Lamine,I Tutusaus,A. Amara,S. Andreon,N. Auricchio,H. Aussel,M. Baldi,S. Bardelli,C. Bodendorf,D. Bonino,E. Branchini,S. Brau-Nogue,M. Brescia,J. Brinchmann,S. Camera,V Capobianco,J. Carretero,S. Casas,M. Castellano,S. Cavuoti,A. Cimatti,G. Congedo,C. J. Conselice,L. Conversi,Y. Copin,F. Courbin,H. M. Courtois,A. Da Silva,H. Degaudenzi,A. M. Di Giorgio,J. Dinis,M. Douspis,F. Dubath,X. Dupac,S. Dusini,A. Ealet,M. Farina,S. Farrens,S. Ferriol,M. Frailis,E. Franceschi,S. Galeotta,W. Gillard,B. Gillis,C. Giocoli,B. R. Granett,A. Grazian,F. Grupp,S. V. H. Haugan,W. Holmes,I Hook,F. Hormuth,A. Hornstrup,P. Hudelot,K. Jahnke,E. Keihanen,S. Kermiche,A. Kiessling,M. Kilbinger,B. Kubik,M. Kuemmel,M. Kunz,H. Kurki-Suonio,S. Ligori,P. B. Lilje,V Lindholm,I Lloro,D. Maino,E. Maiorano,O. Mansutti,O. Marggraf,K. Markovic,N. Martinet,F. Marulli,R. Massey,S. Maurogordato,E. Medinaceli,S. Mei,Y. Mellier,M. Meneghetti,E. Merlin,G. Meylan,M. Moresco,L. Moscardini,E. Munari,S-M Niemi,J. W. Nightingale,C. Padilla,S. Paltani,F. Pasian,K. Pedersen,W. J. Percival,V Pettorino,S. Pires,G. Polenta,M. Poncet,L. A. Popa,L. Pozzetti,F. Raison,R. Rebolo,A. Renzi,J. Rhodes,G. Riccio,E. Romelli,M. Roncarelli,E. Rossetti,R. Saglia,D. Sapone,P. Schneider,A. Secroun,G. Seidel,M. Seiffert,S. Serrano,C. Sirignano,G. Sirri,L. Stanco,C. Surace,P. Tallada-Crespi,D. Tavagnacco,A. N. Taylor,I Tereno,R. Toledo-Moreo,F. Torradeflot,E. A. Valentijn,L. Valenziano,T. Vassallo,A. Veropalumbo,Y. Wang,A. Zacchei,G. Zamorani,J. Zoubian,E. Zucca,A. Biviano,M. Bolzonella,A. Boucaud,E. Bozzo,C. Burigana,C. Colodro-Conde,G. De Lucia,D. Di Ferdinando,J. A. Escartin Vigo,R. Farinelli,J. Gracia-Carpio,G. Mainetti,M. Martinelli,N. Mauri,C. Neissner,Z. Sakr,V Scottez,M. Tenti,M. Viel,M. Wiesmann,Y. Akrami,V Allevato,S. Anselmi,C. Baccigalupi,A. Balaguera-Antolinez,M. Ballardini,L. Blot,S. Borgani,S. Bruton,R. Cabanac,A. Calabro,G. Canas-Herrera,A. Cappi,C. S. Carvalho,G. Castignani,T. Castro,K. C. Chambers,S. Contarini,A. R. Cooray,J. Coupon,S. Davini,B. De Caro,S. de la Torre,G. Desprez,A. Diaz-Sanchez,S. Di Domizio,H. Dole,S. Escoffier,A. G. Ferrari,P. G. Ferreira,I Ferrero,F. Finelli,L. Gabarra,K. Ganga,J. Garcia-Bellido,E. Gaztanaga,F. Giacomini,G. Gozaliasl,H. Hildebrandt,A. Jimenez Munoz,J. J. E. Kajava,V Kansal,D. Karagiannis,C. C. Kirkpatrick,L. Legrand,G. Libet,A. Loureiro,J. Macias-Perez,G. Maggio,M. Magliocchetti,F. Mannucci,R. Maoli,C. J. A. P. Martins,S. Matthew,L. Maurin,R. B. Metcalf,M. Migliaccio,P. Monaco,C. Moretti,G. Morgante,S. Nadathur,N. A. Walton,L. Patrizii,A. Pezzotta,M. Pontinen,V Popa,C. Porciani,D. Potter,I Risso,P-F Rocci,M. Sahlen,A. G. Sanchez,J. A. Schewtschenko,A. Schneider,E. Sefusatti,M. Sereno,J. Steinwagner,N. Tessore,G. Testera,R. Teyssier,S. Toft,S. Tosi,A. Troja,M. Tucci,J. Valiviita,D. Vergani,G. Verza
ASTRONOMY & ASTROPHYSICS（2024）
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Key words
cosmological parameters,dark energy,large-scale structure of Universe
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