COSMOS Team Meeting, Kyoto, 23 May 2005 C-COSMOS The Chandra Cycle 7 COSMOS Proposal Martin Elvis (PI) & 32 others.

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Presentation transcript:

COSMOS Team Meeting, Kyoto, 23 May 2005 C-COSMOS The Chandra Cycle 7 COSMOS Proposal Martin Elvis (PI) & 32 others

COSMOS Team Meeting, Kyoto, 23 May 2005 Strategy: 1/3 of COSMOS field 1.35Msec (out of 3Ms total for Large) 3 years to complete 27 densely tiled observations: large arcsec imaging area 3 x deeper than XMM-Newton: Galaxies Resolves AGN/clusters No ID confusion Low background: stacking XMM field to date XMM structures in Photo-z overdensities Cycle 7 area <2 arcsec hi-res area 0.5sq.deg Cycle 7 200ksec deep area 0.28sq.deg 50ksec wide area 0.64sq.deg Pitch Angle Constraints

COSMOS Team Meeting, Kyoto, 23 May 2005 Science: Emphasize environmental dependencies AGNs as tracers of Large Scale Structure Black Hole Growth in Mergers Starbursts Normal galaxies and stacking analysis Groups & Clusters Radio Source environments AGN SEDs High Redshift & Rare Objects

COSMOS Team Meeting, Kyoto, 23 May 2005 Chandra Cycle 7 TAC Meets June Results by 4th of July?