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20092026
most citedThe WiggleZ Dark Energy Survey: mapping the distance-redshift relation with baryon acoustic oscillations

1k citations · 9.7k across the 121 of their papers we have counts for

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Showing 2019Show all

6 papers · 1 filter

astro-ph.GA2019★ 54 cited

The WiggleZ Dark Energy Survey: Final Data Release and the Metallicity of UV-Luminous Galaxies

Michael J. Drinkwater, Zachary J. Byrne, Chris Blake +24

The WiggleZ Dark Energy Survey measured the redshifts of over 200,000 UV-selected (NUV<22.8 mag) galaxies on the Anglo-Australian Telescope. The survey detected the baryon acoustic…

astro-ph.GA2019★ 29 cited

The effect of gas accretion on the radial gas metallicity profile of simulated galaxies

Florencia Collacchioni, Claudia D. P. Lagos, Peter D. Mitchell +4

We study the effect of the gas accretion rate () on the radial gas metallicity profile (RMP) of galaxies using the EAGLE cosmological hydrodynamic simulations, f…

astro-ph.GA2019★ 150 cited

The KMOS^3D Survey: data release and final survey paper

E. Wisnioski, N. M. Förster Schreiber, M. Fossati +28

We present the completed KMOS survey an integral field spectroscopic survey of 739, , galaxies at using the K-band Multi…

astro-ph.GA2019★ 174 cited

The Evolution and Origin of Ionized Gas Velocity Dispersion from to with KMOS

Hannah D. N. Übler, Reinhard Genzel, Emily Wisnioski +27

We present the evolution of the ionized gas velocity dispersion in 175 star-forming disk galaxies based on data from the full KMOS integral field spectroscop…

astro-ph.GA2019★ 32 cited

Testing Star Formation Laws on Spatially Resolved Regions in a Starburst Galaxy

Piyush Sharda, Elisabete da Cunha, Christoph Federrath +6

We probe the star formation properties of the gas in AzTEC-1 in the COSMOS field, one of the best resolved and brightest starburst galaxies at , forming stars at a r…

astro-ph.GA2019

Size-scaling of clump instabilities in turbulent, feedback regulated disks

Kamran Ali, Danail Obreschkow, Liang Wang +5

We explore the scaling between the size of star-forming clumps and rotational support in massively star-forming galactic disks. The analysis relies on simulations of a clumpy galax…