183 citations · 1.5k across the 34 of their papers we have counts for
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The MOSDEF Survey: Neon as a Probe of ISM Physical Conditions at High Redshift
Moon-Seong Jeong, Alice E. Shapley, Ryan L. Sanders +17
We present results on the properties of neon emission in star-forming galaxies drawn from the MOSFIRE Deep Evolution Field (MOSDEF) survey. Doubly-ionized neon ([NeIII]386…
The MOSDEF Survey: The First Direct Measurements of the Nebular Dust Attenuation Curve at High Redshift
Naveen A. Reddy, Alice E. Shapley, Mariska Kriek +12
We use a sample of 532 star-forming galaxies at redshifts with deep rest-frame optical spectra from the MOSFIRE Deep Evolution Field (MOSDEF) survey to place the fi…
The MOSDEF Survey: An Improved Voronoi Binning Technique on Spatially Resolved Stellar Populations at z~2
Tara Fetherolf, Naveen Reddy, Alice Shapley +12
We use a sample of 350 star-forming galaxies at from the MOSFIRE Deep Evolution Field survey to demonstrate an improved Voronoi binning technique that we use to study…
The MOSDEF Survey: A Comprehensive Analysis of the Rest-optical Emission-line Properties of Star-forming Galaxies
Jordan N. Runco, Alice E. Shapley, Ryan L. Sanders +16
We analyze the rest-optical emission-line spectra of star-forming galaxies in the complete MOSFIRE Deep Evolution Field (MOSDEF) survey. In investigating the origin of t…
The MOSDEF Survey: Differences in SFR and Metallicity for Morphologically-Selected Mergers at z~2
Katelyn Horstman, Alice E. Shapley, Ryan L. Sanders +15
We study the properties of 55 morphologically-identified merging galaxy systems at z~2. These systems are flagged as mergers based on features such as tidal tails, double nuclei, a…
The MOSDEF Survey: the Variation of the Dust Attenuation Curve with Metallicity
Irene Shivaei, Naveen Reddy, George Rieke +14
We derive the UV-optical stellar dust attenuation curve of galaxies at z=1.4-2.6 as a function of gas-phase metallicity. We use a sample of 218 star-forming galaxies, excluding tho…
Towards Studying Hierarchical Assembly in Real Time: A Milky Way Progenitor Galaxy at z = 2.36 under the Microscope
Tom O. Zick, Daniel R. Weisz, Bruno Ribeiro +4
We use Hubble Space Telescope (HST) imaging and near-infrared spectroscopy from Keck/MOSFIRE to study the sub-structure around the progenitor of a Milky Way-mass galaxy in the Hubb…