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The MOSFIRE Deep Evolution Field (MOSDEF) Survey: Rest-Frame Optical Spectroscopy for ~1500 H-Selected Galaxies at 1.37 < z < 3.8
Mariska Kriek, Alice E. Shapley, Naveen A. Reddy +21
In this paper we present the MOSFIRE Deep Evolution Field (MOSDEF) survey. The MOSDEF survey aims to obtain moderate-resolution (R=3000-3650) rest-frame optical spectra (~3700-7000…
On the importance of using appropriate spectral models to derive physical properties of galaxies at 0.7<z<2.8
Camilla Pacifici, Elisabete da Cunha, Stéphane Charlot +14
Interpreting observations of distant galaxies in terms of constraints on physical parameters - such as stellar mass, star-formation rate (SFR) and dust optical depth - requires spe…
Constraining the Low-Mass Slope of the Star Formation Sequence at 0.5<z<2.5
Katherine E. Whitaker, Marijn Franx, Joel Leja +9
We constrain the slope of the star formation rate () to stellar mass () relation down to ($\log(\mathrm{M_{\…
Geometry of Star-Forming Galaxies from SDSS, 3D-HST and CANDELS
A. van der Wel, Yu-Yen Chang, E. F. Bell +18
We determine the intrinsic, 3-dimensional shape distribution of star-forming galaxies at 0<z<2.5, as inferred from their observed projected axis ratios. In the present-day universe…
The Nature of Extreme Emission Line Galaxies at z=1-2: Kinematics and Metallicities from Near-Infrared Spectroscopy
Michael V. Maseda, Arjen van der Wel, Hans-Walter Rix +21
We present near-infrared spectroscopy of a sample of 22 Extreme Emission Line Galaxies at redshifts 1.3 < z < 2.3, confirming that these are low-mass (M* = 10^8 - 10^9 M_sun) galax…
A Massive Galaxy in its Core Formation Phase Three Billion Years After the Big Bang
Erica Nelson, Pieter van Dokkum, Marijn Franx +13
Most massive galaxies are thought to have formed their dense stellar cores at early cosmic epochs. However, cores in their formation phase have not yet been observed. Previous stud…