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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_{\…
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…
Dense cores in galaxies out to z=2.5 in SDSS, UltraVISTA, and the five 3D-HST/CANDELS fields
Pieter van Dokkum, Rachel Bezanson, Arjen van der Wel +15
The dense interiors of massive galaxies are among the most intriguing environments in the Universe. In this paper we ask when these dense cores were formed and determine how galaxi…
3D-HST+CANDELS: The Evolution of the Galaxy Size-Mass Distribution since
A. van der Wel, M. Franx, P. G. van Dokkum +27
Spectroscopic + photometric redshifts, stellar mass estimates, and rest-frame colors from the 3D-HST survey are combined with structural parameter measurements from CANDELS imaging…
3D-HST WFC3-selected Photometric Catalogs in the Five CANDELS/3D-HST Fields: Photometry, Photometric Redshifts and Stellar Masses
Rosalind E. Skelton, Katherine E. Whitaker, Ivelina G. Momcheva +24
The 3D-HST and CANDELS programs have provided WFC3 and ACS spectroscopy and photometry over ~900 square arcminutes in five fields: AEGIS, COSMOS, GOODS-North, GOODS-South, and the…