3.5k citations · 11.5k across the 56 of their papers we have counts for
23 papers · 1 filter
Galaxy And Mass Assembly (GAMA): Testing galaxy formation models through the most massive galaxies in the Universe
P. Oliva-Altamirano, S. Brough, C. Lidman +26
We have analysed the growth of Brightest Group Galaxies and Brightest Cluster Galaxies (BGGs/BCGs) over the last 3 billion years using a large sample of 883 galaxies from the Galax…
Galaxy And Mass Assembly (GAMA): The large scale structure of galaxies and comparison to mock universes
Mehmet Alpaslan, Aaron S. G. Robotham, Simon Driver +18
From a volume limited sample of 45,542 galaxies and 6,000 groups with we use an adapted minimal spanning tree algorithm to identify and classify large scale structur…
Galaxy and Mass Assembly (GAMA): Witnessing the assembly of the cluster Abell 1882
M. S. Owers, I. K. Baldry, A. E. Bauer +14
We present a combined optical and X-ray analysis of the rich cluster Abell 1882 with the aim of identifying merging substructure and understanding the recent assembly history of th…
Galaxy And Mass Assembly (GAMA): Linking Star Formation Histories and Stellar Mass Growth
Amanda E. Bauer, A. M. Hopkins, M. Gunawardhana +23
We present evidence for stochastic star formation histories in low-mass (M* < 10^10 Msun) galaxies from observations within the Galaxy And Mass Assembly (GAMA) survey. For ~73,000…
Galaxy And Mass Assembly (GAMA): A deeper view of the mass, metallicity, and SFR relationships
M. A. Lara-Lopez, A. M. Hopkins, A. R. Lopez-Sanchez +18
A full appreciation of the role played by gas metallicity (Z), star-formation rate (SFR), and stellar mass is fundamental to understanding how galaxies form and evolve. The connect…
Galaxy And Mass Assembly: Evolution of the Halpha luminosity function and star formation rate density up to z<0.35
M. L. P. Gunawardhana, A. M. Hopkins, J. Bland-Hawthorn +28
Measurements of the low-z Halpha luminosity function have a large dispersion in the local number density of sources, and correspondingly in the SFR density. The possible causes for…