597 citations · 6.9k across the 97 of their papers we have counts for
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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…
Bulge-forming galaxies with an extended rotating disk at z~2
Ken-ichi Tadaki, Reinhard Genzel, Tadayuki Kodama +24
We present 0".2-resolution Atacama Large Millimeter/submillimeter Array observations at 870 um for 25 Halpha-seleced star-forming galaxies (SFGs) around the main-sequence at z=2.2-…
The impact of galactic properties and environment on the quenching of central and satellite galaxies: A comparison between SDSS, Illustris and L-Galaxies
Asa F. L. Bluck, J. Trevor Mendel, Sara L. Ellison +7
We quantify the impact that a variety of galactic and environmental properties have on the quenching of star formation. We collate a sample of 400,000 central and 100…
Galaxy pairs in the Sloan Digital Sky Survey - XI. A new method for measuring the influence of the closest companion out to wide separations
David R. Patton, Farid D. Qamar, Sara L. Ellison +5
We describe a statistical approach for measuring the influence that a galaxy's closest companion has on the galaxy's properties out to arbitrarily wide separations. We begin by ide…
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…
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…