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Luminous and High Stellar Mass Candidate Galaxies at z ~ 8 Discovered in CANDELS
Haojing Yan, Steven L. Finkelstein, Kuang-Han Huang +26
One key goal of the Hubble Space Telescope Cosmic Assembly Near-Infrared Deep Extragalactic Legacy Survey is to track galaxy evolution back to z ~ 8. Its two-tiered "wide and deep"…
How Do Star-Forming Galaxies at Z>3 Assemble Their Masses?
Kyoung-Soo Lee, Henry C. Ferguson, Tommy Wiklind +8
We investigate how star-forming galaxies typically assemble their masses at high redshift. Using the deep multi-wavelength coverage of the GOODS dataset, we measure stellar mass of…
Caught in the Act: The Assembly of Massive Cluster Galaxies at z=1.62
J. M. Lotz, C. Papovich, S. M. Faber +13
We present the recent merger history of massive galaxies in a spectroscopically-confirmed proto-cluster at z=1.62. Using HST WFC3 near-infrared imaging from the Cosmic Assembly Nea…
Rest-frame UV--Optically Selected Galaxies at 2.3<z<3.5: Searching for Dusty Star-forming and Passively-Evolving Galaxies
Yicheng Guo, Mauro Giavalisco, Paolo Cassata +17
A new set of color selection criteria (VJL) analogous with the BzK method is designed to select both star-forming galaxies (SFGs) and passively-evolving galaxies (PEGs) at 2.3<z<3.…
CANDELS: The Evolution of Galaxy Rest-Frame Ultraviolet Colors from z = 8 to 4
Steven L. Finkelstein, Casey Papovich, Brett Salmon +18
We study the evolution of galaxy rest-frame ultraviolet (UV) colors in the epoch 4 < z < 8. We use new wide-field near-infrared data in GOODS-S from the CANDELS, HUDF09 and ERS pro…
Galaxy Structure and Mode of Star Formation in the SFR-Mass Plane from z ~ 2.5 to z ~ 0.1
Stijn Wuyts, Natascha M. Forster Schreiber, Arjen van der Wel +23
We analyze the dependence of galaxy structure (size and Sersic index) and mode of star formation (Σ_SFR and SFR_IR/SFR_UV) on the position of galaxies in the SFR versus Mass diagra…