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The MOSDEF Survey: [SIII] as a New Probe of Evolving ISM Conditions
Ryan L. Sanders, Tucker Jones, Alice E. Shapley +15
We present measurements of [SIII]9069,9531 for a sample of star-forming galaxies, the first sample with measurements of these lines at z>0.1. We employ the line rati…
Half-mass radii of quiescent and star-forming galaxies evolve slowly from 0 < z < 2.5: implications for galaxy assembly histories
Katherine A. Suess, Mariska Kriek, Sedona H. Price +1
We use high-resolution, multi-band imaging of ~16,500 galaxies in the CANDELS fields at 0 < z < 2.5 to study the evolution of color gradients and half-mass radii over cosmic time.…
The SFR-radius connection: data and implications for wind strength and halo concentration
Lin Lin, S. M. Faber, David C. Koo +26
This paper is one in a series that explores the importance of radius as a second parameter in galaxy evolution. The topic investigated here is the relationship between star formati…
The MOSDEF Survey: The Metallicity Dependence of X-ray Binary Populations at
Francesca M. Fornasini, Mariska Kriek, Ryan L. Sanders +15
Population synthesis models predict that high-mass X-ray binary (HMXB) populations produced in low metallicity environments should be more X-ray luminous, a trend supported by stud…
Quenching as a Contest between Galaxy Halos and their Central Black Holes
Zhu Chen, S. M. Faber, David. C. Koo +27
Existing models of galaxy formation have not yet explained striking correlations between structure and star-formation activity in galaxies, notably the sloped and moving boundaries…
The MOSDEF Survey: Sulfur Emission-line Ratios Provide New Insights into Evolving ISM Conditions at High Redshift
Alice E. Shapley, Ryan L. Sanders, Peng Shao +15
We present results on the emission-line properties of 1.3<=z<=2.7 galaxies drawn from the complete MOSFIRE Deep Evolution Field (MOSDEF) survey. Specifically, we use observations o…