activity
20122020
most citedGalaxy And Mass Assembly (GAMA): The galaxy stellar mass function to from the r-band selected equatorial regions

135 citations · 614 across the 9 of their papers we have counts for

collaborators

18 papers

astro-ph.GA202021 cited

Galaxy and Mass Assembly: luminosity and stellar mass functions in GAMA groups

J. A. Vázquez-Mata, J. Loveday, S. D. Riggs +14

How do galaxy properties (such as stellar mass, luminosity, star formation rate, and morphology) and their evolution depend on the mass of their host dark matter halo? Using the Ga…

astro-ph.GA2020

Mergers Do Trigger AGNs out to z 0.6

F. Gao, L. Wang, W. J. Pearson +6

Aims. The fueling and feedback of Active Galactic Nuclei (AGNs) are important in understanding the co-evolution between black holes and host galaxies. Mergers are thought to have t…

astro-ph.GA2019109 cited

The WISE Extended Source Catalogue (WXSC) I: The 100 Largest Galaxies

T. H. Jarrett, M. E. Cluver, M. J. I. Brown +3

We present mid-infrared photometry and measured global properties of the 100 largest galaxies in the sky, including the Magellanic Clouds, Local Group galaxies M31 and M33, the For…

astro-ph.GA201922 cited

Galaxy And Mass Assembly (GAMA): Properties and evolution of red spiral galaxies

Smriti Mahajan, Kriti Kamal Gupta, Rahul Rana +10

We use multi-wavelength data from the Galaxy and Mass Assembly (GAMA) survey to explore the cause of red optical colours in nearby (0.002<z<0.06) spiral galaxies. We show that the…

astro-ph.GA201966 cited

4MOST Consortium Survey 7: Wide-Area VISTA Extragalactic Survey (WAVES)

S. P. Driver, J. Liske, L. J. M. Davies +12

WAVES is designed to study the growth of structure, mass and energy on scales of ~1 kpc to ~10 Mpc over a 7 Gyr timeline. On the largest length scales (1-10 Mpc) WAVES will measure…

astro-ph.GA2018

Galaxy And Mass Assembly (GAMA): The sSFR-M* relation part I - -M* as a function of sample, SFR indicator and environment

L. J. M. Davies, C. del P. Lagos, A. Katsianis +11

Recently a number of studies have proposed that the dispersion along the star formation rate - stellar mass relation (-M) is indicative of variations in st…