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19952026
most citedGalaxy and Mass Assembly (GAMA): survey diagnostics and core data release

1.1k citations · 24k across the 302 of their papers we have counts for

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Showing 2019 · astro-ph.GAShow all

15 papers · 2 filters

astro-ph.GA2019★ 9 cited

The SAMI Galaxy Survey: The contribution of different kinematic classes to the stellar mass function of nearby galaxies

Kexin Guo, Luca Cortese, Danail Obreschkow +10

We use the complete Sydney-AAO Multi-object Integral field spectrograph (SAMI) Galaxy Survey to determine the contribution of slow rotators, as well as different types of fast rota…

astro-ph.GA2019★ 20 cited

Star-gas misalignment in galaxies: I. The properties of galaxies from the Horizon-AGN simulation and comparisons to SAMI

Donghyeon J. Khim, Sukyoung K. Yi, Yohan Dubois +12

Recent integral field spectroscopy observations have found that about 11% of galaxies show star-gas misalignment. The misalignment possibly results from external effects such as ga…

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★ 6 cited

The SAMI Galaxy Survey: rules of behaviour for spin-ellipticity radial tracks in galaxies

Alexander Rawlings, Caroline Foster, Jesse van de Sande +18

We study the behaviour of the spin-ellipticity radial tracks for 507 galaxies from the Sydney AAO Multi-object Integral Field (SAMI) Galaxy Survey with stellar kinematics out to $\…

astro-ph.GA2019★ 94 cited

The SAMI Galaxy Survey: First detection of a transition in spin orientation with respect to cosmic filaments in the stellar kinematics of galaxies

C. Welker, J. Bland-Hawthorn, J. Van de Sande +16

We present the first detection of mass dependent galactic spin alignments with local cosmic filaments with over 2 sigma confidence using IFS kinematics. The 3D network of cosmic fi…

astro-ph.GA2019★ 30 cited

The SAMI Galaxy Survey: mass-kinematics scaling relations

Dilyar Barat, Francesco D'Eugenio, Matthew Colless +17

We use data from the Sydney-AAO Multi-object Integral-field spectroscopy (SAMI) Galaxy Survey to study the dynamical scaling relation between galaxy stellar mass and the gene…

astro-ph.GA2019★ 72 cited

The Close AGN Reference Survey (CARS). A massive multi-phase outflow impacting the edge-on galaxy HE1353-1917

B. Husemann, J. Scharwächter, T. A. Davis +15

[Abridged] We combine extensive spatially-resolved multi-wavelength observations, taken as part of the Close AGN Reference Survey (CARS), for the edge-on disc galaxy HE1353-1917 to…

astro-ph.GA2019★ 14 cited

The Close AGN Reference Survey (CARS). Discovery of a global [CII] 158 m line excess in AGN HE1353-1917

I. Smirnova-Pinchukova, B. Husemann, G. Busch +15

The [CII]158m line is one of the strongest far-infrared (FIR) lines and an important coolant in the interstellar medium of galaxies that is accessible out to high redshifts. The…

astro-ph.GA2019★ 31 cited

The Close AGN Reference Survey (CARS): Comparative analysis of the structural properties of star-forming and non-star-forming galaxy bars

Justus Neumann, Dimitri A. Gadotti, Lutz Wisotzki +12

The absence of star formation in the bar region that has been reported for some galaxies can theoretically be explained by shear. However, it is not clear how star-forming (SF) bar…

astro-ph.GA2019★ 7 cited

Assembly bias evidence in close galaxy pairs

Ignacio Ferreras, Andrew M. Hopkins, Claudia Lagos +4

The growth channel of massive galaxies involving mergers can be studied via close pairs as putative merger progenitors, where the stellar populations of the satellite galaxies will…

astro-ph.GA2019★ 45 cited

The SAMI Galaxy Survey: Stellar population radial gradients in early-type galaxies

I. Ferreras, N. Scott, F. La Barbera +16

We study the internal radial gradients of the stellar populations in a sample comprising 522 early-type galaxies (ETGs) from the SAMI (Sydney- AAO Multi-object Integral field spect…

astro-ph.GA2019★ 23 cited

4MOST Consortium Survey 6: Active Galactic Nuclei

A. Merloni, D. A. Alexander, M. Banerji +17

X-ray and mid-infrared emission are signposts of the accretion of matter onto the supermassive black holes that reside at the centres of most galaxies. As a major step towards unde…

astro-ph.GA2019★ 18 cited

The SAMI Galaxy Survey: Bayesian Inference for Gas Disk Kinematics using a Hierarchical Gaussian Mixture Model

Mathew R. Varidel, Scott M. Croom, Geraint F. Lewis +20

We present a novel Bayesian method, referred to as Blobby3D, to infer gas kinematics that mitigates the effects of beam smearing for observations using Integral Field Spectroscopy…

astro-ph.GA2019★ 42 cited

The SAMI Galaxy Survey: Satellite galaxies undergo little structural change during their quenching phase

L. Cortese, J. van de Sande, C. P. Lagos +9

At fixed stellar mass, satellite galaxies show higher passive fractions than centrals, suggesting that environment is directly quenching their star formation. Here, we investigate…

astro-ph.GA2019★ 81 cited

The SAMI Galaxy Survey: Quenching of star formation in clusters I. Transition galaxies

Matt S. Owers, Michael J. Hudson, Kyle A. Oman +19

We use integral field spectroscopy from the SAMI Galaxy Survey to identify galaxies that show evidence for recent quenching of star formation. The galaxies exhibit strong Balmer ab…