Philippe Fischer

The Mass Distribution of the Most Luminous X-Ray Cluster RXJ 1347.5-1145 From Gravitational Lensing

Galaxy cluster mass distribution are potentially useful probes of

The Carina dwarf spheroidal galaxy - How dark is it?

\Omega_0

Mass Segregation in Young Large Magellanic Cloud Clusters. I. NGC 2157

and the nature of the dark matter. Large clusters will distort the observed shapes of background galaxies through gravitational lensing allowing the measurement of the cluster mass distributions. In this paper we describe weak statistical lensing measurements of the most luminous X-ray cluster known, RXJ1347.5-1145 at z=0.45. We detect a shear signal in the background galaxies at a signal-to-noise ratio of 7.5 in the radial range

A kinematic study of the Fornax dwarf spheroidal galaxy

120 \le r \le 1360 h^{-1}

Weak-Lensing Measurements of 42 SDSS/RASS Galaxy Clusters

kpc. A mass map of the cluster reveals an 11

The Mass Distribution of the Cluster 0957+561 From Gravitational Lensing

\sigma

Nonparametric dynamical analysis of globular clusters: M15, 47 TUC, NGC 362, and NGC 3201

peak in the cluster mass distribution consistent with the position of the central dominant galaxy and 3

A search for binaries in the globular cluster NGC 3201

\sigma

Dynamics of the young LMC cluster NGC 1866

evidence for the presence of a subcluster at a projected radius of 1.3 - 1.7 h^{-1} Mpc from the cluster center. In the range

Discovery of a New Quadruple Lens HST 1411+5211* **

120 \le r \le 1360 h^{-1}