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High Velocity Dispersion in A Rare Grand Design Spiral Galaxy at Redshift z=2.18
David R. Law, Alice E. Shapley, Charles C. Steidel +3
Although relatively common in the local Universe, only one grand-design spiral galaxy has been spectroscopically confirmed to lie at z>2 (HDFX 28; z=2.011), and may prove to be a m…
An HST/WFC3-IR Morphological Survey of Galaxies at z = 1.5-3.6: II. The Relation between Morphology and Gas-Phase Kinematics
David R. Law, Charles C. Steidel, Alice E. Shapley +3
We analyze rest-frame optical morphologies and gas-phase kinematics as traced by rest-frame far-UV and optical spectra for a sample of 204 star forming galaxies in the redshift ran…
The Characteristic Star Formation Histories of Galaxies at Redshifts z~2-7
Naveen A. Reddy, Max Pettini, Charles C. Steidel +3
A large sample of spectroscopically confirmed galaxies at 1.4<z<3.7, with complementary imaging in the near- and mid-IR from the ground and from Hubble and Spitzer, is used to infe…
The Gaseous Environment of High-z Galaxies: Precision Measurements of Neutral Hydrogen in the Circumgalactic Medium of z ~ 2-3 Galaxies in the Keck Baryonic Structure Survey
Gwen C. Rudie, Charles C. Steidel, Ryan F. Trainor +7
We present results from the Keck Baryonic Structure Survey (KBSS), a unique spectroscopic survey designed to explore the connection between galaxies and intergalactic baryons. The…
An HST/WFC3-IR Morphological Survey of Galaxies at z = 1.5-3.6: I. Survey Description and Morphological Properties of Star Forming Galaxies
David R. Law, Charles C. Steidel, Alice E. Shapley +3
We present the results of a 42-orbit HST/WFC3 survey of the rest-frame optical morphologies of star forming galaxies with spectroscopic redshifts in the range z=1.5-3.6. The survey…
The Mass-Radius Relation for Star-Forming Galaxies at z ~ 1.5-3.0
Sarah R. Nagy, David R. Law, Alice E. Shapley +1
We present early results from a Hubble Space Telescope (HST) WFC3/IR imaging survey of star-forming galaxies in the redshift range 1.5 < z < 3.0. When complete, this survey will co…