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Borgani, S. |
Volume |
Paper Title |
Page Number |
Authors |
51 |
Hierarchical Statistics and Fractal Structure |
186 |
Borgani, S. |
94 |
CDM--like VS CHDM Models: the Distribution of Galaxy Clusters |
283 |
Borgani, S. |
94 |
The Cluster Velocity Field |
289 |
Moscardini, L.; Branchini, E.; Brunozzi, P. Tini; Borgani, S.; Plionis, M.; Coles, P. |
176 |
The Local Cluster Mass Function from Optical Virial Analysis |
28 |
Girardi, M.; Boschin, W.; Giuricin, G.; Mardirossian, F.; Mezzetti, M.; Borgani, S. |
200 |
Tracing the Evolution of the Cluster Abundance |
210 |
Borgani, S. |
200 |
Confirming EIS Clusters. Multi-Object Spectroscopy |
390 |
Biviano, A.; Ramella, M.; Boschin, W.; Bardelli, S.; Scodeggio, M.; da Costa, L.N.; Olsen, L. F.; Nonino, M.; Borgani, S.; Girardi, M. |
234 |
The Chandra Deep Field South: Preliminary X-ray and Optical Results |
525 |
Giacconi, R.; Rosati, P.; Tozzi, P.; Nonino, M.; Hasinger, G.; Norman, C.; Bergeron, J.; Borgani, S.; Gilli, R.; Gilmozzi, R.; Zheng, W. |
268 |
Evolution of the Cluster Population with the ROSAT Deep Cluster Survey |
31 |
Borgani, S.; Rosati, P. |
268 |
X-Ray Temperature and Morphology of z>0.8 Clusters of Galaxies |
35 |
Holden, B.; Stanford, S. A.; Rosati, P.; Tozzi, P.; Squires, G.; Borgani, S.; Eisenhardt, P. |
453 |
Hydrodynamic Simulations with the Godunov SPH |
259 |
Borgani, S.; Murante, G.; Brunino, R.; Cha, S.-H. |
521 |
Shall Numerical Astrophysics Step Into the Era of Exascale Computing? |
567 |
Taffoni, G.; Murante, G.; Tornatore, L.; Goz, D.; Borgani, S.; Katevenis, M.; Chrysos, N.; Marazakis, M. |
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