426 citations · 4.3k across the 76 of their papers we have counts for
12 papers · 1 filter
The distribution of stellar orbits in Eagle galaxies -- the effect of mergers, gas accretion, and secular evolution
Giulia Santucci, Claudia Del P. Lagos, Katherine E. Harborne +9
The merger history of a galaxy is thought to be one of the major factors determining its internal dynamics, with galaxies having undergone different types or mergers (e.g. dry, min…
SimSpin v2.6.0 -- Constructing synthetic spectral IFU cubes for comparison with observational surveys
K. E. Harborne, A. Serene, E. J. A. Davies +10
In this work, we present a methodology and a corresponding code-base for constructing mock integral field spectrograph (IFS) observations of simulated galaxies in a consistent and…
Identifying the discs, bulges, and intra-halo light of simulated galaxies through structural decomposition
Katy L. Proctor, Claudia del P. Lagos, Aaron D. Ludlow +1
We perform a structural decomposition of galaxies identified in three cosmological hydrodynamical simulations by applying Gaussian Mixture Models (GMMs) to the kinematics of their…
Resolving cosmic star formation histories of present-day bulges, disks, and spheroids with ProFuse
Sabine Bellstedt, Aaron S. G. Robotham, Simon P. Driver +3
We present the first look at star formation histories of galaxy components using ProFuse, a new technique to model the 2D distribution of light across multiple wavelengths using si…
Unbiased surveys of dust-enshrouded galaxies using ALMA
K. Kohno, S. Fujimoto, A. Tsujita +43
The ALMA lensing cluster survey (ALCS) is a 96-hr large program dedicated to uncovering and characterizing intrinsically faint continuum sources and line emitters with the assistan…
Galaxy And Mass Assembly (GAMA): The group HI mass as a function of halo mass
Ajay Dev, Simon P. Driver, Martin Meyer +11
We determine the atomic hydrogen (HI) to halo mass relation (HIHM) using Arecibo Legacy Fast ALFA survey HI data at the location of optically selected groups from the Galaxy and Ma…
The Spitzer Extragalactic Representative Volume Survey and DeepDrill extension: clustering of near-infrared galaxies
Eelco van Kampen, Mark Lacy, Duncan Farrah +7
We have measured the angular auto-correlation function of near-infrared galaxies in SERVS+DeepDrill, the Spitzer Extragalactic Representative Volume Survey and its follow-up survey…
Evolution in the orbital structure of quiescent galaxies from MAGPI, LEGA-C and SAMI surveys: direct evidence for merger-driven growth over the last 7 Gy
Francesco D'Eugenio, Arjen van der Wel, Joanna M. Piotrowska +37
We present the first study of spatially integrated higher-order stellar kinematics over cosmic time. We use deep rest-frame optical spectroscopy of quiescent galaxies at redshifts…
Different higher-order kinematics between star-forming and quiescent galaxies based on the SAMI, MAGPI and LEGA-C surveys
Francesco D'Eugenio, Arjen van der Wel, Caro Derkenne +38
We present the first statistical study of spatially integrated non-Gaussian stellar kinematics spanning 7 Gyr in cosmic time. We use deep, rest-frame optical spectroscopy of massiv…
Exploring the Intrinsic Scatter of the Star-Forming Galaxy Main Sequence at redshift 0.5 to 3.0
Rongjun Huang, Andrew J. Battisti, Kathryn Grasha +4
Previous studies have shown that the normalization and scatter of the galaxy 'main sequence' (MS), the relation between star formation rate (SFR) and stellar mass (), evolves…
The cosmic radio background from 150 MHz--8.4 GHz, and its division into AGN and star-forming galaxy flux
Scott A. Tompkins, Simon P. Driver, Aaron S. G. Robotham +4
We present a revised measurement of the extra-galactic background light (EBL) at radio frequencies based on a near complete compendium of radio source counts. We present the radio-…
Galaxy quenching timescales from a forensic reconstruction of their colour evolution
Matías Bravo, Aaron S. G. Robotham, Claudia del P. Lagos +3
The timescales on which galaxies move out of the blue cloud to the red sequence () provide insight into the mechanisms driving quenching. Here, we build upon previ…