activity
20162026
most citedGalaxy And Mass Assembly (GAMA): Data Release 4 and the z < 0.1 total and z < 0.08 morphological galaxy stellar mass functions

249 citations · 1.4k across the 40 of their papers we have counts for

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Showing 2017Show all

8 papers · 1 filter

astro-ph.GA201730 cited

Galaxy And Mass Assembly: Automatic Morphological Classification of Galaxies Using Statistical Learning

Sreevarsha Sreejith, Sergiy Pereverzyev, Lee S. Kelvin +15

We apply four statistical learning methods to a sample of galaxies () from the Galaxy and Mass Assembly (GAMA) survey to test the feasibility of using automated algo…

astro-ph.GA201732 cited

Galaxy And Mass Assembly (GAMA): The Consistency of GAMA and WISE Derived Mass-to-Light Ratios

T. Kettlety, J. Hesling, S. Phillipps +11

Recent work has suggested that mid-IR wavelengths are optimal for estimating the mass-to-light ratios of stellar populations and hence the stellar masses of galaxies. We compare st…

astro-ph.GA201783 cited

Galaxy And Mass Assembly (GAMA): The mechanisms for quiescent galaxy formation at

K. Rowlands, V. Wild, N. Bourne +14

One key problem in astrophysics is understanding how and why galaxies switch off their star formation, building the quiescent population that we observe in the local Universe. From…

astro-ph.GA201746 cited

HST imaging of the brightest z~8-9 galaxies from UltraVISTA: the extreme bright end of the UV luminosity function

Mauro Stefanon, Ivo Labbé, Rychard J. Bouwens +13

We report on the discovery of three especially bright candidate galaxies. Five sources were targeted for follow-up with HST/WFC3, selected from a larger sample…

astro-ph.GA2017128 cited

The abundance of ultra-diffuse galaxies from groups to clusters: UDGs are relatively more common in more massive haloes

Remco F. J. van der Burg, Henk Hoekstra, Adam Muzzin +17

In recent years, multiple studies have reported substantial populations of large, low-surface-brightness galaxies in local galaxy clusters. Various theories that aim to explain the…

astro-ph.GA201720 cited

Galaxy And Mass Assembly: the evolution of the cosmic spectral energy distribution from z = 1 to z = 0

Stephen K. Andrews, Simon P. Driver, Luke J. M. Davies +15

We present the evolution of the Cosmic Spectral Energy Distribution (CSED) from . Our CSEDs originate from stacking individual spectral energy distribution fits based on…