LAM oca fermilab

INSU


CeSAM
Observations organization page

The DAFT/FADA team is lead by Mel Ulmer 1, Doug Clowe 2 and Cristophe Adami 3

The Team includes:

S. Allam 4, C. Benoist 5, A.Biviano 6A. Cappi 7, Cristiano DaRocha 16,17, F. Durret 8 , C.Ferrari 5 , R. Gavazzi 8, L. Guennou 3,18, O. Ilbert 3, V. Le Brun 3, G. Lima Neto 14, H. Lin 4, I. Marquez 13, P. Marshall 9,10, S. Maurogordato 5, K. Murphy 2, H. Plana 15, F. Rostagni 5, T. Schrabback 12, E. Slezak 5, D.Tucker 4, S. Arnouts 3, S. Basa 3, J.G. Cuby 3, J.P. Kneib 3, R. Malina 3, A. Mazure 3, D. Russeil 3, C. Schimd 3

1 Department Physics & Astronomy, Northwestern University
2 Department of Physics and Astronomy, Ohio University
3 Laboratoire d'Astrophysique de Marseille (CNRS/INSU and Université Aix-Marseille)
4 Fermi National Accelerator Laboratory
5 Laboratoire Cassiopée (Observatoire de la Côte d'Azur /CNRS)
6 INAF/Osservatorio Astronomico di Trieste
7 INAF - Osservatorio Astronomico di Bologna
8 Institut d'Astrophysique de Paris (CNRS/INSU and Université Pierre et Marie Curie)
9 Kavli Institute for Particle Astrophysics and Cosmology, Stanford University
10 Physics Department, University of California, Santa Barbara
12 Leiden Observatory, Leiden University
13 Instituto de Astrofisica de Andalucia (CSIC), Spain
14 Institute of Astronomy, Geophysics and Atmospheric Sciences, University of São Paolo, Brazil
15 State University of Santa Cruz, Ilhéus, Brazil
16 Núcleo de Astrofísica Teórica, Universidade Cruzeiro do Sul, Brazil
17 European Southern Observatory, Garching
18 Institut d'Astrophysique Spatiale, Orsay
Ph. D. Thesis :
- L. Guennou (LAM)  :  Line of sight caracterization and photometric redshifts
- K. Murphy (Ohio University)  :  Weak lensing tomography
- N. Martinet (IAP)  :  Weak lensing analysis of HST DAFT/FADAS images
- R. Santana (Ohio University)  :  Weak lensing tomography