Articles citing this article

The Citing articles tool gives a list of articles citing the current article.
The citing articles come from EDP Sciences database, as well as other publishers participating in CrossRef Cited-by Linking Program. You can set up your personal account to receive an email alert each time this article is cited by a new article (see the menu on the right-hand side of the abstract page).

Cited article:

Tomographic cluster clustering as a cosmological probe

M. Romanello, F. Marulli, L. Moscardini, C. Giocoli, G. F. Lesci, S. Contarini, A. Fumagalli and B. Sartoris
Astronomy & Astrophysics 693 A195 (2025)
https://doi.org/10.1051/0004-6361/202451566

Euclid preparation

L. Ingoglia, M. Sereno, S. Farrens, C. Giocoli, L. Baumont, G. F. Lesci, L. Moscardini, C. Murray, M. Vannier, A. Biviano, C. Carbone, G. Covone, G. Despali, M. Maturi, S. Maurogordato, M. Meneghetti, M. Radovich, B. Altieri, A. Amara, S. Andreon, N. Auricchio, C. Baccigalupi, M. Baldi, S. Bardelli, F. Bellagamba, et al.
Astronomy & Astrophysics 695 A280 (2025)
https://doi.org/10.1051/0004-6361/202452122

Euclid preparation

M. Sereno, S. Farrens, L. Ingoglia, G. F. Lesci, L. Baumont, G. Covone, C. Giocoli, F. Marulli, S. Miranda La Hera, M. Vannier, A. Biviano, S. Maurogordato, L. Moscardini, N. Aghanim, S. Andreon, N. Auricchio, M. Baldi, S. Bardelli, F. Bellagamba, C. Bodendorf, D. Bonino, E. Branchini, M. Brescia, J. Brinchmann, S. Camera, et al.
Astronomy & Astrophysics 689 A252 (2024)
https://doi.org/10.1051/0004-6361/202348680

SPT clusters with DES and HST weak lensing. II. Cosmological constraints from the abundance of massive halos

S. Bocquet, S. Grandis, L. E. Bleem, M. Klein, J. J. Mohr, T. Schrabback, T. M. C. Abbott, P. A. R. Ade, M. Aguena, A. Alarcon, S. Allam, S. W. Allen, O. Alves, A. Amon, A. J. Anderson, J. Annis, B. Ansarinejad, J. E. Austermann, S. Avila, D. Bacon, M. Bayliss, J. A. Beall, K. Bechtol, M. R. Becker, A. N. Bender, et al.
Physical Review D 110 (8) (2024)
https://doi.org/10.1103/PhysRevD.110.083510