Astronomy and Astrophysics – Astronomy
Scientific paper
Jan 2009
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aas...21333405c&link_type=abstract
American Astronomical Society, AAS Meeting #213, #334.05; Bulletin of the American Astronomical Society, Vol. 41, p.395
Astronomy and Astrophysics
Astronomy
Scientific paper
We study galaxy masses and colors at 0 < z < 1.2 using new deep imaging with the Subaru Telescope of the MUSYC Extended Chandra Deep Field South. We detect 80,000 galaxies with photometric redshifts out to z=5.0 in our catalog with RAB > 27. We obtain photometric redshifts with the accuracy to better than 2% (Δ z / (1+ z) \sim 0.01, z < 1.2) using EAZY, a fast public photometric redshift code. Using deep X-ray observations from Chandra we detect 1000 AGN and derive their host galaxy masses and star formation histories. We compare the AGN host galaxies to the general galaxy population.
This work was made possible by support from Chandra observer award #SP8-9002X, NSF grant #AST0407295 and Spitzer JPL Grant #RSA1288440.
Brammer Gabriel
Cardamone Carolin N.
Gawiser Eric
Kriek Mariska
Sasaki Satoshi
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