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20082025
most cited3D-HST+CANDELS: The Evolution of the Galaxy Size-Mass Distribution since

1.4k citations · 18.9k across the 155 of their papers we have counts for

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Showing 2016Show all

8 papers · 1 filter

astro-ph.GA2016★ 108 cited

Galaxy environment in the 3D-HST fields. Witnessing the onset of satellite quenching at z ~ 1-2

M. Fossati, D. J. Wilman, J. T. Mendel +25

We make publicly available a catalog of calibrated environmental measures for galaxies in the five 3D-HST/CANDELS deep fields. Leveraging the spectroscopic and grism redshifts from…

astro-ph.GA2016★ 135 cited

Predicting Quiescence: The Dependence of Specific Star Formation Rate on Galaxy Size and Central Density at 0.5<z<2.5

Katherine E. Whitaker, Rachel Bezanson, Pieter G. van Dokkum +9

In this paper, we investigate the relationship between star formation and structure, using a mass-complete sample of 27,893 galaxies at selected from 3D-HST. We confirm…

astro-ph.GA2016★ 21 cited

The Relation Between [OIII]/H and Specific Star Formation Rate in Galaxies at

Claire Mackay Dickey, Pieter van Dokkum, Pascal Oesch +7

Recent surveys have identified a seemingly ubiquitous population of galaxies with elevated [OIII]/H emission line ratios at , though the nature of this phenomenon continu…

astro-ph.GA2016★ 32 cited

Ages of massive galaxies at from 3D-HST rest-frame optical spectroscopy

Mattia Fumagalli, Marijn Franx, Pieter van Dokkum +10

We present low-resolution near-infrared stacked spectra from the 3D-HST survey up to and fit them with commonly used stellar population synthesis models: BC03 (Bruzual & Ch…

astro-ph.GA2016★ 136 cited

The evolution of metallicity and metallicity gradients from z=2.7-0.6 with KMOS3D

Eva Wuyts, Emily Wisnioski, Matteo Fossati +28

We present measurements of the [NII]/Ha ratio as a probe of gas-phase oxygen abundance for a sample of 419 star-forming galaxies at z=0.6-2.7 from the KMOS3D near-IR multi-IFU surv…

astro-ph.GA2016★ 122 cited

KMOS^3D: Dynamical constraints on the mass budget in early star-forming disks

S. Wuyts, N. M. Förster Schreiber, E. Wisnioski +26

We exploit deep integral-field spectroscopic observations with KMOS/VLT of 240 star-forming disks at 0.6 < z < 2.6 to dynamically constrain their mass budget. Our sample consists o…