I am interested in the properties of dark matter halos, from galaxy to cluster scales. The main tools i use are gravitational lensing and N-body simulations

Weak Galaxy-Galaxy Lensing in Clusters

A New Window of Exploration in the Mass Spectrum: Strong Lensing BY Galaxy Groups in the SL2S

Combining Strong and Weak Gravitational Lensing in Abell 1689

Probing the Truncation of Galaxy Dark Matter Halos in High Density Environments from Hydrodynamical N-body Simulations

Probing the Slope of Cluster Mass Profile with Gravitational Rings: Application to Abell 1689

Strong Lensing in Abell 1703: Constraints on the Slope of the Inner Dark Matter Distribution

Where is the matter in the Merging Cluster Abell 2218 ?

Mapping Dark Matter in Galaxy Clusters: From Weak Galaxy-Galaxy Lensing to Cluster Lensing

Full Publications

Teaching: advanced cosmology course for master students:

details (plan of the course + lecture: Gravitational Lensing as a probe of Dark Matter halos)

Cluster Lensing bibliography:

details