AAS 205th Meeting, 9-13 January 2005
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All findings are embargoed until the time of presentation at the meeting.


Session 72. First Results from HST Cosmic Evolution Survey

Special Session, Tuesday, January 11, 2005, 10:00-11:30am, Town and Country

Associated Posters in Session 61.
72.01 COSMOS -- Cosmic Evolution Survey
N. Scoville (Caltech), COSMOS Team
72.02 The COSMOS HST/ACS Observations: A Public Legacy
A. M. Koekemoer (STScI), COSMOS Team
72.03 Star Formation Rate as a Function of Environment and Morphology
B. Mobasher, D. Calzetti (STScI), N. Scoville (Caltech), E. Schinnerer (MPE-HD)
72.04 COSMOS: Clustering evolution from z=1.5
O. Le Fevre (LAM- Marseille, France), L. Guzzo (OABr , Milan, Italy), B. Meneux (LAM-Marseille, France), A. Pollo (OABr, Milan, Italy), N. Scoville (Caltech), J.P. Kneib (LAM-Marseille, France), COSMOS Collaboration
72.05 Dark Matter Maps with Cosmos
J.D. Rhodes (JPL), COSMOS Weak Lensing Team
72.06 The VLA 1.4 GHz Survey of the COSMOS field
E. Schinnerer (MPIA), C.L. Carilli (NRAO), N.Z. Scoville (Caltech), COSMOS/VLA-COSMOS Collaboration
72.07 GALEX and COSMOS: Morphologies of star forming galaxies out to z~1
D. Schiminovich, M. Zamojski (Columbia University), R. M. Rich (UCLA), HST COSMOS Team, GALEX Science Team
72.08 Evolution of AGN in the cosmic web: The XMM-Newton Cosmos Survey
I. Lehmann, G. Hasinger, H. Boehringer, H. Brunner, M. Brusa (MPE Garching), A. Comastri (Osservatorio Astronomico di Bologna), M. Elvis (Harvard-Smithsonian Center for Astrophysics), A. Finoguenov (MPE Garching), F. Fiore (Osservatorio Astronomico di Roma), A. Franceschini (Universitadi Padova), R. Gilli (NAF, Firenze), R. Griffiths (Carnegie Mellon University), C. Impey (University of Arizona), O. Le'Fevre (Laboratoire d'Astrophysique de Marseille), S. Lilly (ETH Zurich), V. Mainieri (MPE Garching), G. Matt (Universitadegli Studi Roma Tre), I. Matute (MPE Garching), T. Miyaji (Carnegie Mellon University), S. Molendi (IASF-CNR, Milano), S. Paltani (Laboratoire d'Astrophysique de Marseille), D. Sanders (University of Hawaii), N. Scoville (California Institute of Technology), L. Tresse (Laboratoire d'Astrophysique de Marseille), M. Urry (Yale University), G. Vettolani (Istituto di Radioastronomia, CNR Bologna), G. Zamorani (Osservatorio Astronomico di Bologna)


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