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20032025
most cited3D-HST+CANDELS: The Evolution of the Galaxy Size-Mass Distribution since

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astro-ph.CO2013

The Morphologies of Massive Galaxies at 1 < z < 3 in the CANDELS-UDS Field

V. A. Bruce, J. S. Dunlop, M. Cirasuolo +16

We have used high-resolution, HST WFC3/IR, near-infrared imaging to conduct a detailed bulge-disk decomposition of the morphologies of ~200 of the most massive (M_star > 10^11 M_so…