Final Agenda
(23^rd March 2002)

Sunday March 17th
30'	-	General introduction J. Peebles (Princeton) - Transparencies - Postscript
Morning Session: Expansion (SN - H0) Chairman J. Steinberger (CERN)
30'	-	History G. Tammann (Basel) - Transparencies - Postscript
30'	-	Distance scales - HST W. Freedman (Pasadena) - Transparencies - Postscript
30'	-	Age of the Universe B. Chaboyer (Dartmouth) - Transparencies - Postscript
15'	-	H0 from CBI P. Udomprasert (Pasadena) - Transparencies - Postscript
15'	-	Surface brightness S. Mei (Orsay) - Transparencies - Postscript
Afternoon Session 1 : Cosmic Microwave Background (1) Chairman S. White (Munich)
30'	-	Pre-history of CMB Studies B. Partridge (Haverford) - Transparencies - Postscript
20'	-	CMB Observations in the Planck Era F. Bouchet (Paris) - Transparencies - Postscript
20'	-	CMB Observations in the Post-Planck Era J. Peterson (Pittsburgh) - Transparencies - Postscript
Afternoon Session 2 : Nucleosynthesis (1) Chairman S. White (Munich)
20'	-	Deuterium with Fuse G. Hebrard (Paris) - Transparencies - Postscript
40'	-	BBN: theoretical inputs and uncertainties, comparison with the deuterium observations in QSO's S. Burles (Boston) - Transparencies - Postscript
20'	-	Lithium-7: evolution S. Vauclair (Toulouse) - Transparencies - Postscript

Monday March 18th

Morning Session: The nature of dark matter (1) Chairman S. Borgani (Trieste)

30'	-	Baryonic dark matter J. Silk (Oxford) - Transparencies - Postscript
30'	-	Non-baryonic dark matter R. Kolb (Cern) - Transparencies - Postscript
30'	-	Direct and indirect detection G. Chardin (Saclay) - Transparencies - Postscript
15'	-	Matter density in clusters A. Mahdavi (Hawaii) - Transparencies - Postscript
Afternoom Session 1 : Nucleosynthesis (2) Chairman J. Silk (Oxford)
40'	-	Helium-3 observations / galactic evolution T. Bania (Boston) - Transparencies - Postscript
30'	-	Helium-4 V. Luridiana (Mexico) - Transparencies - Postscript
Afternoom Session 2 : Cosmic Microwave Background (2) Chairman J. Silk (Oxford)
15'	-	Testing gaussianity of the CMB: MAXIMA A. Heavens (Edimburgh) - Transparencies - Postscript
15'	-	Tools to Detect non-Gaussianity in non-standard Cosmological Models J.-L. Sanz (Santander) - Transparencies - Postscript
15'	-	An update on the study of CMB Gaussianity J.-H. Wu (Berkeley) - Postscript
15'	-	Gaussianity of the CMB maps S. Shandarin (Kansas) - Transparencies - Postscript
15'	-	Galactic foregrounds for the Very Small Array at 30 GHz C. Dickinson (Manchester) - Transparencies - Postscript
15'	-	Varying alpha in the early universe: CMB, large-scale structure and Fisher matrix analysis C. Martins (Cambridge) - Transparencies - Postscript

Tuesday March 19th
Morning Session 1 : Primordial Universe (1) Chairman D. Lyth (Lancaster)
30'	-	Brane cosmology - review D. Langlois (Paris) - Transparencies - Postscript
15'	-	Cosmological brane perturbations K. Malik (Paris) - Transparencies - Postscript
15'	-	Brane cosmology with a bulk scalar field M. Rodriguez-Martinez (Paris) - Transparencies - Postscript
Morning Session 2 : Structure Formation (1) Chairman D. Lyth (Lancaster)
40'	-	Structure formation - Review S. White (Garching) - Transparencies - Postscript
15'	-	Local Group Velocity M. Chodorowski (Warsaw) - Transparencies - Postscript
15'	-	Hubble Flow C. Horellou (Onsala) - Transparencies - Postscript
15'	-	Cosmological parameters from LSS V. Lukash (Moscow) - Transparencies - Postscript
Afternoon Session 1 : Galaxy Distribution Chairman F. Bouchet (Paris)
30'	-	Extraction of cosmological parameters O. Lahav (Cambridge) - Transparencies - Postscript
15'	-	The topology of the 2dF galaxies A. Canavezes (Cambridge) - Transparencies - Postscript
15'	-	Bias of galaxies L. Verde (Princeton) - Transparencies - Postscript
15'	-	HDF survey S. Arnouts (ESO) - Transparencies - Postscript
15'	-	Clustering - VVDS and CFDF S. Foucaud (Marseille) - Transparencies - Postscript
15'	-	DEEP2 C. Marinoni (Berkeley) - Transparencies - Postscript
Afternoon Session 2 : The nature of dark matter (2) Chairman F. Bouchet (Paris)
15'	-	Probing dark matter distribution with gravitational lensing and stellar dynamics T. Treu (Pasadena) - Transparencies - Postscript
15'	-	The self-annihilation signal from cold dark matter J. Taylor (Oxford) - Transparencies - Postscript
15'	-	Detecting Dark Matter Substructure with Strong Gravitational Lenses B. Metcalf (Cambridge) - Transparencies - Postscript

Wednesday March 20th
Morning Session 1 : Clusters (1) Chairman R. Fusco-Femiano (Roma)
40'	-	Clusters as Cosmic Probes A. Blanchard (Toulouse) - Transparencies - Postscript
15'	-	AMI M. Jones (Cambridge) - Transparencies - Postscript
15'	-	Cosmological constraints from SZ R. Kneissl (Cambridge) - Transparencies - Postscript
15'	-	SZ Survey Simulations J. Geisbuesch (Cambridge) - Transparencies - Postscript
Morning Session 2 : Primordial Universe (2) Chairman R. Fusco-Femiano (Roma)
15'	-	A braneworld cosmology from colliding bubbles M. Bucher (Cambridge) - Transparencies - Postscript
15'	-	Perturbations in the Ekpyrotic Scenarios P. Peter (Paris) - Transparencies - Postscript
15'	-	Baryogenesis M. Gleiser (Dartmouth) - Transparencies - Postscript
15'	-	Loop corrections to quintessence potentials J. Jackel (Heidelberg) - Transparencies - Postscript
Afternoon Session 1 : Weak Lensing Chairman Ch. Balland (Orsay)
30'	-	Review of observational results L. Van Waerbeke (Paris) - Transparencies - Postscript
15'	-	Weak lensing effects in quintessence models K. Benabed (New-York) - Postscript
15'	-	Gravitational mass profiles S. Ettori (ESO) - Transparencies - Postscript
15'	-	Numerical arc cross sections M. Meneghetti (Padova) - Transparencies - Postscript
15'	-	S-Z and weak lensing Ph. Marshall (Cavendish) - Transparencies - Postscript
Afternoon Session 2 : The cosmological constant and dark energy (1) Chairman Ch. Balland (Orsay)
15'	-	Possibilities for future supernovae and cluster survey to probe dark energy J. Weller (Cambridge) - Transparencies - Postscript
15'	-	Nature of dark energy I. Maor (Beer-Sheva) - Transparencies - Postscript
15'	-	A not-so-constant cosmological constant? M. Kunz (Oxford) - Transparencies - Postscript
15'	-	About the cosmological constant? R. Triay (Oxford) - Transparencies - Postscript

Thursday March 21st
Morning Session 1 : The cosmological constant and dark energy (2) Chairman W. Freedman (Pasadena)
30'	-	Supernovae N. Regnault (Berkeley) - Transparencies - Postscript
15'	-	Constraints on dark energy R. Bean (London) - Transparencies - Postscript
15'	-	Measurement of high-z SN1a J. Raux (Paris) - Transparencies - Postscript
15'	-	The Supernova Factory project P. Antilogus (Lyon) - Transparencies - Postscript
15'	-	Coupling dark energy with dark matter L. Amendola (Roma) - Transparencies - Postscript
Morning Session 2 : Structure Formation (2) Chairman W. Freedman (Pasadena)
15'	-	Dark energy and structure formation J. Schwindt (Heidelberg) - Transparencies - Postscript
15'	-	Primordial magnetic field M. Langer (Orsay) - Transparencies - Postscript
15'	-	Cluster masses in simulations A. Maccio (Milano) - Transparencies - Postscript
15'	-	Recent dynamical evolution of clusters and Omega_m M. Plionis (Athens) - Transparencies - Postscript
Afternoon Session : Cosmic Microwave Background (3) Chairman K. Gorski (ESO)
15'	-	Analysing interferometric CMB data K. Maisinger (Cambridge) - Transparencies - Postscript
15'	-	First results from the VSA K. Grainge (Cambridge) - Transparencies - Postscript
15'	-	The VSA power spectrum and Cosmological Implications A. Taylor (Cambridge) - Transparencies not allowed to be posted on the web - Postscript
15'	-	The VSA power spectrum and Cosmological Implications R. Savage (Cambridge) - Transparencies not allowed to be posted on the web - Postscript
15'	-	Measurements of the CMB Power Spectrum to L=3500 with the CBI B. Mason (Pasadena) - Transparencies - Postscript
15'	-	Cosmology from BOOMERANG and CBI C. Contaldi (Toronto) - Transparencies not allowed to be posted on the web - Postscript
15'	-	Archeops A. Amblard (Paris) - Transparencies - Postscript
15'	-	CMB data analysis M. Douspis (Oxford) - Transparencies - Postscript
15'	-	CMBEASY, intuitivly calculating the CMB M. Doran (Heidelberg) - Transparencies - Postscript

Friday March 22nd
Morning Session 1 : Primordial Universe (3) Chairman R. Kolb (CERN)
30'	-	Inflation - review D. Lyth (Lancaster) - Transparencies - Postscript
15'	-	Support for inflation from the pre-Planck era A. Gangui (Buenos-Aires) - Transparencies - Postscript
15'	-	Lambda-inflation versus observation E. Mikheeva (Moscow) - Transparencies - Postscript
15'	-	Generalized chaotic inflation F. Cao (Paris) - Transparencies - Postscript
Morning Session 2 : Cosmic Microwave Background (4) Chairman R. Kolb (CERN)
15'	-	The COBE legacy K. Gorski (ESO) - Postscript
15'	-	What can we learn from CMB polarization measurements ? J. Delabrouille (Paris) - Transparencies - Postscript
15'	-	CMB polarization and CBI J. Cartwright (Pasadena) - Transparencies - Postscript
Afternoon Session 1 : Clusters (2) Chairman G. Tammann (Basel)
15'	-	Strong Lensing Clusters G. Golse (Toulouse) - Transparencies - Postscript
15'	-	Wide Field Imaging C. Ferrari (Nice) - Transparencies - Postscript
15'	-	Detection of SZ clusters D. Herranz (Santander) - Transparencies - Postscript
15'	-	Superclusters with SZ surveys A. Diaferio (Torino) - Transparencies - Postscript
15'	-	Estimating z of galaxy clusters from SZE data J. Diego Rodriguez (Oxford) - Transparencies - Postscript
15'	-	Heating and cooling the ICM S. Borgani (Trieste) - Transparencies - Postscript
15'	-	Dark matter vs baryons in clusters N. Menci (Bologna) - Transparencies - Postscript
15'	-	Iron abundances in hydrodynamical SPH simulations of galaxy clusters R. Valdarnini (Trieste) - Transparencies - Postscript
15'	-	Lens magnification by CL0024+1654 in U and R: constraints on cluster mass and the faint U band field galaxy number count slope S. Dye (London) - Transparencies - Postscript

Saturday March 23rd
Closing session Summary Talk Chairman J. Tran Thanh Van (Orsay)
45'	-	Summary talk O. Lahav (London) - Transparencies - Postscript