Testing gravity on large scales. The skewness of the galaxy distribution at z~1
| dc.creator | Marinoni, C. | |
| dc.creator | Guzzo, L. | |
| dc.creator | Cappi, A. | |
| dc.creator | Fevre, O. Le | |
| dc.creator | Mazure, A. | |
| dc.creator | Meneux, B. | |
| dc.creator | Pollo, A. | |
| dc.creator | Iovino, A. | |
| dc.creator | McCracken, H. J. | |
| dc.creator | Scaramella, R. | |
| dc.creator | de la Torre, S. | |
| dc.creator | Virey, J. M. | |
| dc.creator | Bottini, D. | |
| dc.creator | Garilli, B. | |
| dc.creator | Brun, V. Le | |
| dc.creator | Maccagni, D. | |
| dc.creator | Picat, J. P. | |
| dc.creator | Scodeggio, M. | |
| dc.creator | Tresse, L. | |
| dc.creator | Vettolani, G. | |
| dc.creator | Zanichelli, A. | |
| dc.creator | Adami, C. | |
| dc.creator | Arnouts, S. | |
| dc.creator | Bardelli, S. | |
| dc.creator | Bolzonella, M. | |
| dc.creator | Charlot, S. | |
| dc.creator | Ciliegi, P. | |
| dc.creator | Contini, T. | |
| dc.creator | Foucaud, S. | |
| dc.creator | Franzetti, P. | |
| dc.creator | Gavignaud, I. | |
| dc.creator | Ilbert, O. | |
| dc.creator | Lamareille, F. | |
| dc.creator | Marano, B. | |
| dc.creator | Mathez, G. | |
| dc.creator | Merighi, R. | |
| dc.creator | Paltani, S. | |
| dc.creator | Pellò, R. | |
| dc.creator | Pozzetti, L. | |
| dc.creator | Radovich, M. | |
| dc.creator | Vergani, D. | |
| dc.creator | Zamorani, G. | |
| dc.creator | Zucca, E. | |
| dc.creator | Abbas, U. | |
| dc.creator | Bondi, M. | |
| dc.creator | Bongiorno, A. | |
| dc.creator | Brinchmann, J. | |
| dc.creator | Buzzi, A. | |
| dc.creator | Cucciati, O. | |
| dc.creator | de Ravel, L. | |
| dc.creator | Gregorini, L. | |
| dc.creator | Mellier, Y. | |
| dc.creator | Merluzzi, P. | |
| dc.creator | Perez-Montero, E. | |
| dc.creator | Taxil, P. | |
| dc.creator | Temporin, S. | |
| dc.creator | Walcher, C. J. | |
| dc.date | 2008-11-14 | |
| dc.date.accessioned | 2026-07-07T10:18:26Z | |
| dc.date.available | 2026-07-07T10:18:26Z | |
| dc.description | We study the evolution of the low-order moments of the galaxy overdensity distribution over the redshift interval 0.7<z<1.5. We find that the variance and the normalized skewness evolve over this redshift interval in a way that is remarkably consistent with predictions of first- and second-order perturbation theory. This finding confirms the standard gravitational instability paradigm over nearly 9 Gyrs of cosmic time and demonstrates the importance of accounting for the non-linear component of galaxy biasing to avoid disagreement between theory and observations. | |
| dc.description | To appear in the proceedings of 43rd Rencontres de Moriond on Cosmology (La Thuile, 2008) | |
| dc.identifier | https://arxiv.org/abs/0811.2358 | |
| dc.identifier | http://arxiv.org/abs/0811.2358 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/174188 | |
| dc.subject | Astrophysics | |
| dc.title | Testing gravity on large scales. The skewness of the galaxy distribution at z~1 | |
| dc.type | text |