most citedConstraining the Low-Mass Slope of the Star Formation Sequence at 0.5<z<2.5

871 citations · 2.1k across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2014★ 265 cited

The Formation of Massive, Compact Galaxies at z=2 in the Illustris Simulation

Sarah Wellons, Paul Torrey, Chung-Pei Ma +13

Massive, quiescent galaxies at high redshift have been found to be considerably more compact than galaxies of similar mass in the local universe. How these compact galaxies formed…

astro-ph.GA2014★ 597 cited

The KMOS^3D Survey: design, first results, and the evolution of galaxy kinematics from 0.7<z<2.7

E. Wisnioski, N. M. Förster Schreiber, S. Wuyts +24

We present the KMOS^3D survey, a new integral field survey of over 600 galaxies at 0.7<z<2.7 using KMOS at the Very Large Telescope (VLT). The KMOS^3D survey utilizes synergies wit…

astro-ph.GA2014★ 871 cited

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_{\…

astro-ph.GA2014★ 136 cited

A Consistent Study of Metallicity Evolution at 0.8 < z < 2.6

Eva Wuyts, Jaron Kurk, Natascha M. Förster Schreiber +33

We present the correlations between stellar mass, star formation rate (SFR) and [NII]/Ha flux ratio as indicator of gas-phase metallicity for a sample of 222 galaxies at 0.8 < z <…

astro-ph.GA2014★ 89 cited

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…

astro-ph.GA2014★ 139 cited

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…