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ZFOURGE/CANDELS: On the Evolution of M* Galaxy Progenitors from z=3 to 0.5
Casey Papovich, I. Labbé, R. Quadri +38
Galaxies with stellar masses near M* contain the majority of stellar mass in the universe, and are therefore of special interest in the study of galaxy evolution. The Milky Way (MW…
Modeling the Initial Conditions of Interacting Galaxy Pairs Using Identikit
S. Alireza Mortazavi, Jennifer M. Lotz, Joshua E. Barnes +1
We develop and test an automated technique to model the dynamics of interacting galaxy pairs. We use Identikit (Barnes & Hibbard 2009, Barnes 2011) as a tool for modeling and match…
Diverse Structural Evolution at z > 1 in Cosmologically Simulated Galaxies
Gregory F. Snyder, Jennifer Lotz, Christopher Moody +5
From mock Hubble Space Telescope images, we quantify non-parametric statistics of galaxy morphology, thereby predicting the emergence of relationships among stellar mass, star form…
No More Active Galactic Nuclei in Clumpy Disks Than in Smooth Galaxies at z~2 in CANDELS / 3D-HST
Jonathan R. Trump, Guillermo Barro, Stephanie Juneau +23
We use CANDELS imaging, 3D-HST spectroscopy, and Chandra X-ray data to investigate if active galactic nuclei (AGNs) are preferentially fueled by violent disk instabilities funnelin…
CANDELS Visual Classifications: Scheme, Data Release, and First Results
Jeyhan S. Kartaltepe, Mark Mozena, Dale Kocevski +49
We have undertaken an ambitious program to visually classify all galaxies in the five CANDELS fields down to H<24.5 involving the dedicated efforts of 65 individual classifiers. On…