Slide 1CDFS SA12 SA15 Morphologies & Star Formation Histories of Massive Galaxies at z > 1.3 P. McCarthy & The GDDS Team Venice 2006 Slide 2 Star Formation Histories…

Slide 1To measure the brightness distribution of galaxies, we must determine the surface brightness of the resolved galaxy. Surface brightness = magnitude within 1 square…

Slide 1 Unveiling the properties of distant stellar populations Michele Cantiello INAF Osservatorio Astronomico di Teramo - Italy Collaborators @ INAF-Osservatorio Astronomico…

Slide 1 time space Cosmic bullet temperature Slide 2 Slide 3 Another look at dark halos J. Dubinski Toronto/CITA New big cosmo simulations Halos vs. Elliptical Galaxies –deVaucouleurs…

Slide 1 Elliptical galaxies appear simple: roundish on the sky, the light is smoothly distributed, and they lack star formation patches or strong internal obscuration by…

The 2dF galaxy redshift survey John Peacock & the 2dFGRS team Harvard, October 1999 Outline Brief history 2dF Survey motivation & design Survey data Spectral classification…

Elliptical galaxies appear simple: roundish on the sky, the light is smoothly distributed, and they lack star formation patches or strong internal obscuration by dust. But…

J. Cohen, Concepcion, Feb 2006 Part 1 â the very young GCs in M31, already published: ApJL (Nov 2005) Part 2 â integrated light photometry of Galactic GCs (ready for publication…