Now showing items 1-3 of 3

  • Alam, Shadab; Ata, Metin; Bailey, Stephen; Beutler, Florian; Bizyaev, Dmitry; Blazek, Jonathan A; Bolton, Adam S.; Brownstein, Joel R.; Burden, Angela; Chuang, Chia-Hsun; Comparat, Johan; Cuesta, Antonio J.; Dawson, Kyle S; Eisenstein, Daniel J.; Escoffier, Stephanie; Gil-Marin, Hector; Grieb, Jan Niklas; Hand, Nick; Ho, Shirley; Kinemuchi, Karen; Kirkby, David; Kitaura, Francisco; Malanushenko, Elena; Malanushenko, Viktor; Maraston, Claudia; McBride, Cameron K.; Nichol, Robert C.; Olmstead, Matthew D.; Oravetz, Daniel J; Padmanabhan, Nikhil; Palanque-Delabrouille, Nathalie; Pan, Kaike; Pellejero-Ibanez, M; Percival, Will J.; Petitjean, Patrick; Prada, Francisco; Price-Whelan, Adrian M; Reid, Beth A.; Rodríguez-Torres, Sergio A.; Roe, Natalie A; Ross, Ashley J.; Ross, Nicholas P.; Rossi, Graziano; Rubiño-Martín, J. A.; Saito, Shun; Salazar-Albornoz, Salvador; Samushia, Lado; Sanchez, Ariel G.; Satpathy, Siddharth; Schlegel, David J.; Schneider, Donald P; Scoccola, Claudia G; Seo, Hee-Jong; Sheldon, Erin S; Simmons, Audrey; Slosar, Anze; Strauss, Michael A; Swanson, Molly E C; Thomas, Daniel; Tinker, Jeremy L; Tojeiro, Rita; Magana, Mariana Vargas; Vazquez, Jose Alberto; Verde, Licia; Wake, David A; Wang, Yuting; Weinberg, David H; White, Martin; Wood-Vasey, W Michael; Yeche, Christophe; Zehavi, Idit; Zhai, Zhongxu; Zhao, Gong-Bo (Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2017)
    We present cosmological results from the final galaxy clustering data set of the Baryon Oscillation Spectroscopic Survey, part of the Sloan Digital Sky Survey III. Our combined galaxy sample comprises 1.2 million massive ...
  • Guglielmo, Valentina; Saglia, R.; Castander, F. J.; Galametz, A.; Paltani, S.; Bender, R.; Bolzonella, M.; Capak, Peter L.; Ilbert, O.; Masters, D. C.; Stern, D.; Andreon, S.; Auricchio, N.; Balaguera-Antolinez, A.; Baldi, Marco; Bardelli, S.; Biviano, A.; Bodendorf, C.; Bonino, D.; Bozzo, E.; Branchini, Enzo; Brau-Nogue, S.; Brescia, Massimo; Burigana, C.; Cabanac, R A; Camera, S.; Capobianco, V.; Cappi, A.; Carbone, Carmelita; Carretero, J.; Carvalho, C. S.; Casas, R.; Casas, S.; Castellano, M.; Castignani, G.; Cavuoti, S.; Cimatti, Andrea; Clédassou, Rodolphe; Colodro-Conde, Carlos; Congedo, G.; Conselice, C. J.; Conversi, L.; Copin, Y.; Corcione, L.; Costille, A.; Coupon, J.; Courtois, H. M.; Cropper, Mark; Da Silva, A.; de la Torre, S.; Di Ferdinando, D.; Dubath, F.; Duncan, C. A. J.; Dupac, X.; Dusini, S.; Fabricius, M.; Farrens, S.; Ferreira, Pedro G.; Fotopoulou, S.; Frailis, M.; Franceschi, E.; Fumana, M.; Galeotta, S.; Garilli, B.; Gillis, B.; Giocoli, C.; Gozaliasl, Ghassem; Graciá-Carpio, J.; Grupp, F.; Guzzo, Luigi; Hildebrandt, Helmut; Hoekstra, Henk; Hormuth, F.; Israel, H.; Jahnke, Knud; Keihänen, Elina; Kermiche, S.; Kilbinger, M.; Kirkpatrick, C. C.; Kitching, Thomas D.; Kubik, B.; Kunz, Martin; Kurki-Suonio, Hannu; Laureijs, R.; Ligori, S.; Lilje, Per Barth; Lloro, Ivan; Maino, Davide; Maiorano, E.; Maraston, Claudia; Marggraf, O.; Martinet, N.; Marulli, F.; Massey, R.; Maurogordato, S.; Medinaceli, E.; Mei, S.; Meneghetti, M.; Metcalf, R. Benton; Meylan, G.; Moresco, M.; Moscardini, L.; Munari, E.; Nakajima, R.; Neissner, C.; Niemi, S.; Nucita, A. A.; Padilla, C.; Pasian, F.; Patrizii, L; Pocino, A.; Poncet, M.; Pozzetti, L.; Raison, F.; Renzi, A.; Rhodes, Jason D.; Riccio, G.; Romelli, E; Roncarelli, M.; Rossetti, E.; Sánchez, A. G.; Sapone, D.; Schneider, Peter; Scottez, V.; Secroun, A.; Serrano, S.; Sirignano, C.; Sirri, G.; Sureau, F.; Tallada-Crespí, P.; Tavagnacco, Daniele; Taylor, A. N.; Tenti, M.; Tereno, I.; Toledo-Moreo, Rafael; Torradeflot, F.; Tramacere, A.; Valenziano, L.; Vassallo, T.; Wang, Y.; Welikala, N; Wetzstein, M.; Whittaker, L.; Zacchei, Andrea; Zamorani, G.; Zoubian, J.; Zucca, E. (Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2020)
    The Complete Calibration of the Colour–Redshift Relation survey (C3R2) is a spectroscopic effort involving ESO and Keck facilities designed specifically to empirically calibrate the galaxy colour–redshift relation – P ( z ...
  • Bisigello, Laura; Kuchner, U.; Conselice, C. J.; Andreon, S.; Bolzonella, M.; Duc, P.-A.; Garilli, B.; Humphrey, A.; Maraston, Claudia; Moresco, M.; Pozzetti, L.; Tortora, C.; Zamorani, G.; Auricchio, N.; Brinchmann, Jarle; Capobianco, V.; Carretero, J.; Castander, F. J.; Castellano, M.; Cavuoti, S.; Cimatti, Andrea; Clédassou, Rodolphe; Congedo, G.; Conversi, L.; Corcione, L.; Cropper, Mark S.; Dusini, S.; Frailis, M.; Franceschi, E.; Franzetti, P.; Fumana, M.; Hormuth, F.; Israel, H.; Jahnke, Knud; Kermiche, S.; Kitching, Thomas D.; Kohley, R.; Kubik, B.; Kunz, Martin; Le Fèvre, Olivier; Ligori, S.; Lilje, Per Barth; Lloro, Ivan; Maiorano, E.; Marggraf, O.; Massey, R.; Masters, D. C.; Mei, S.; Mellier, Yannick; Meylan, G.; Padilla, C.; Paltani, S.; Pasian, F.; Pettorino, V.; Pires, S.; Polenta, G.; Poncet, M.; Raison, F.; Rhodes, Jason D.; Roncarelli, M.; Rossetti, E.; Saglia, R.; Sauvage, M.; Schneider, Peter; Secroun, A.; Serrano, S.; Sureau, F.; Taylor, A. N.; Tereno, I.; Toledo-Moreo, Rafael; Valenziano, L.; Wang, Y.; Wetzstein, M.; Zoubian, J. (Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2020)
    The Euclid mission will observe well over a billion galaxies out to z ∼ 6 and beyond. This will offer an unrivalled opportunity to investigate several key questions for understanding galaxy formation and evolution. The ...