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The First Robust Constraints on the Relationship Between Dust-to-Gas Ratio and Metallicity in Luminous Star-forming Galaxies at High Redshift
Alice E. Shapley, Fergus Cullen, James S. Dunlop +4
We present rest-optical spectroscopic properties of a sample of four galaxies in the Atacama Large Millimeter/submillimeter Array Hubble Ultra Deep Field (ALMA HUDF). These galaxie…
The MOSDEF-LRIS Survey: The Connection Between Massive Stars and Ionized Gas in Individual Galaxies at
Michael W. Topping, Alice E. Shapley, Naveen A. Reddy +5
We present constraints on the massive star and ionized gas properties for a sample of 62 star-forming galaxies at . Using BPASS stellar population models, we fit the rest…
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 Mass-Metallicity Relation at z=8: Direct-Method Metallicity Constraints and Near-Future Prospects
Tucker Jones, Ryan Sanders, Guido Roberts-Borsani +4
Physical properties of galaxies at z>7 are of interest for understanding both the early phases of star formation and the process of cosmic reionization. Chemical abundance measurem…
Kinematics of the Circumgalactic Medium of a Galaxy from MgII Tomography
Kris Mortensen, Keerthi Vasan G. C., Tucker Jones +5
Galaxy evolution is thought to be driven in large part by the flow of gas between galaxies and the circumgalactic medium (CGM), a halo of metal-enriched gas extending out to $\gtrs…
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…