666 citations · 7.1k across the 83 of their papers we have counts for
8 papers · 1 filter
First test of Verlinde's theory of Emergent Gravity using Weak Gravitational Lensing measurements
Margot M. Brouwer, Manus R. Visser, Andrej Dvornik +19
Verlinde (2016) proposed that the observed excess gravity in galaxies and clusters is the consequence of Emergent Gravity (EG). In this theory the standard gravitational laws are m…
Galaxy-Galaxy Lensing in EAGLE: comparison with data from 180 square degrees of the KiDS and GAMA surveys
Marco Velliscig, Marcello Cacciato, Henk Hoekstra +14
We present predictions for the galaxy-galaxy lensing profile from the EAGLE hydrodynamical cosmological simulation at redshift z=0.18, in the spatial range 0.02 < R/(Mpc/h) < 2, an…
Galaxy And Mass Assembly (GAMA): Active Galactic Nuclei in Pairs of Galaxies
Yjan A. Gordon, Matt S. Owers, Kevin A. Pimbblet +14
There exist conflicting observations on whether or not the environment of broad and narrow line AGN differ and this consequently questions the validity of the AGN unification model…
Galaxy and Mass Assembly (GAMA): Exploring the WISE Cosmic Web in G12
T. H. Jarrett, M. E. Cluver, C. Magoulas +17
We present an analysis of the mid-infrared WISE sources seen within the equatorial GAMA G12 field, located in the North Galactic Cap. Our motivation is to study and characterize th…
A consistent model for both the HI and stellar mass functions of galaxies
Hazel Martindale, Peter A. Thomas, Bruno M. Henriques +1
Using the L-Galaxies semi-analytic model we simultaneously fit the HI mass function, stellar mass function and galaxy colours. We find good fits to all three observations at z = 0…
GAMA/H-ATLAS: A meta-analysis of SFR indicators - comprehensive measures of the SFR-M* relation and Cosmic Star Formation History at z < 0.4
L. J. M. Davies, S. P. Driver, A. S. G. Robotham +26
We present a meta-analysis of star-formation rate (SFR) indicators in the GAMA survey, producing 12 different SFR metrics and determining the SFR-M* relation for each. We compare a…