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  • Adam, R.; Vannier, M.; Maurogordato, S.; Biviano, A.; Adami, C.; Ascaso, B.; Bellagamba, F.; Benoist, C.; Cappi, A.; Díaz-Sánchez, A.; Durret, F.; Farrens, S.; Gonzalez, A. H.; Iovino, A.; Licitra, R.; Maturi, M.; Mei, S.; Merson, A.; Munari, E.; Pelló, R.; Ricci, M.; Rocci, P. F.; Roncarelli, M.; Sarron, F.; Amoura, Y.; Andreon, S.; Apostolakos, N.; Arnaud, M.; Bardelli, S.; Bartlett, J.; Baugh, C. M.; Borgani, S.; Brodwin, M.; Castander, F.; Castignani, G.; Cucciati, O.; De Lucia, G.; Dubath, P.; Fosalba, P.; Giocoli, C.; Hoekstra, Henk; Mamon, G. A.; Melin, J. B.; Moscardini, L.; Paltani, S.; Radovich, M.; Sartoris, B.; Schultheis, M.; Sereno, M.; Weller, Jochen; Burigana, C.; Carvalho, C. S.; Corcione, L.; Kurki-Suonio, Hannu; Lilje, Per Barth; Sirri, G.; Toledo-Moreo, Rafael; Zamorani, G. (Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2019)
    Galaxy cluster counts in bins of mass and redshift have been shown to be a competitive probe to test cosmological models. This method requires an efficient blind detection of clusters from surveys with a well-known selection ...