Shannon G. Patel, Pieter G. van Dokkum, Marijn Franx, Ryan F. Quadri, Adam Muzzin, Danilo Marchesini, Rik J. Williams, Bradford P. Holden, Mauro Stefanon
We study the structural evolution of massive galaxies by linking progenitors and descendants at a constant cumulative number density of n_c=1.4x10^{-4} Mpc^{-3} to z\sim3. Structural parameters were measured by fitting Sersic profiles to high resolution CANDELS HST WFC3 J_{125} and H_{160} imaging in the UKIDSS-UDS at 1View original: http://arxiv.org/abs/1208.0341
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