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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_{\…
Reconciling the observed star-forming sequence with the observed stellar mass function
Joel Leja, Pieter van Dokkum, Marijn Franx +1
We examine the connection between the observed star-forming sequence (SFR ) and the observed evolution of the stellar mass function between . We find…
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…
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…