594 citations · 5.7k across the 89 of their papers we have counts for
11 papers · 2 filters
Modelling the cosmic spectral energy distribution and extragalactic background light over all time
Stephen K. Andrews, Simon P. Driver, Luke J. Davies +2
We present a phenomological model of the Cosmic Spectral Energy Distribution (CSED) and the integrated galactic light (IGL) over all cosmic time. This model, based on an earlier mo…
GAMA/G10-COSMOS/3D-HST: The 0<z<5 cosmic star-formation history, stellar- and dust-mass densities
Simon P. Driver, Stephen K. Andrews, Elisabete da Cunha +30
We use the energy-balance code MAGPHYS to determine stellar and dust masses, and dust corrected star-formation rates for over 200,000 GAMA galaxies, 170,000 G10-COSMOS galaxies and…
Galactic googly: the rotation-metallicity bias in the inner stellar halo of the Milky Way
Prajwal R. Kafle, Sanjib Sharma, Aaron S. G. Robotham +4
The first and second moments of stellar velocities encode important information about the formation history of the Galactic halo. However, due to the lack of tangential motion and…
VALES: I. The molecular gas content in star-forming dusty H-ATLAS galaxies up to z=0.35
V. Villanueva, E. Ibar, T. M. Hughes +24
We present an extragalactic survey using observations from the Atacama Large Millimeter/submillimeter Array (ALMA) to characterise galaxy populations up to : the Valparaíso…
Radio observations confirm young stellar populations in local analogues to Lyman break galaxies
Stephanie M. L. Greis, Elizabeth R. Stanway, Andrew J. Levan +2
We present radio observations at 1.5 GHz of 32 local objects selected to reproduce the physical properties of star-forming galaxies. We also report non-detections of five…
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…
Galaxy And Mass Assembly (GAMA): The galaxy stellar mass function to from the r-band selected equatorial regions
A. H. Wright, A. S. G. Robotham, S. P. Driver +23
We derive the low redshift galaxy stellar mass function (GSMF), inclusive of dust corrections, for the equatorial Galaxy And Mass Assembly (GAMA) dataset covering 180 deg. We c…
Galaxy and Mass Assembly (GAMA): Probing the merger histories of massive galaxies via stellar populations
I. Ferreras, A. M. Hopkins, M. L. P. Gunawardhana +13
The merging history of galaxies can be traced with studies of dynamically close pairs. These consist of a massive primary galaxy and a less massive secondary (or satellite) galaxy.…
Galaxy and Mass Assembly (GAMA): Formation and Growth of Elliptical Galaxies in the Group Environment
Simon Deeley, Michael J. Drinkwater, Daniel Cunnama +16
There are many proposed mechanisms driving the morphological transformation of disk galaxies to elliptical galaxies. In this paper, we determine if the observed transformation in l…
VALES: III. The calibration between the dust continuum and interstellar gas content of star-forming galaxies
T. M. Hughes, E. Ibar, V. Villanueva +23
We present the calibration between the dust continuum luminosity and interstellar gas content obtained from the Valparaíso ALMA Line Emission Survey (VALES) sample of 67 main-seque…
Galaxy And Mass Assembly: The 1.4GHz SFR indicator, SFR-M* relation and predictions for ASKAP-GAMA
L. J. M. Davies, M. T. Huynh, A. M. Hopkins +20
We present a robust calibration of the 1.4GHz radio continuum star formation rate (SFR) using a combination of the Galaxy And Mass Assembly (GAMA) survey and the Faint Images of th…