249 citations · 733 across the 20 of their papers we have counts for
20 papers
The role of gas stripping in the quenching of satellite galaxies using SHARK v2.0
Megan K. Oxland, Matías Bravo, Laura C. Parker +1
Observational studies have made substantial progress in characterizing quenching as a function of stellar mass and environment, but they are often limited in their ability to const…
The galaxy-AGN scaling relations over 13 billion years in SHARK v2.0 (I): SMBH masses
Matías Bravo, Claudia del P. Lagos, Katy L. Proctor +2
The presence of strong correlations between super-massive black hole (SMBH) masses and galaxy properties like stellar mass have been well-established in the local Universe, but how…
Deep Extragalactic VIsible Legacy Survey (DEVILS): New robust merger rates at intermediate redshifts
Melissa F. Fuentealba-Fuentes, Luke J. M. Davies, Aaron S. G. Robotham +5
Mergers are fundamental to our understanding of the processes driving the evolution of the structure and morphology of galaxies, star formation, AGN activity, and the redistributio…
ALMACAL XIII. Evolution of the CO luminosity function and the molecular gas mass density out to ~ 6
Victoria Bollo, Céline Péroux, Martin Zwaan +7
Cold molecular gas, largely traced by CO emission, is the primary fuel for star formation, making it essential for understanding galaxy evolution. ALMA has made significant progres…
The MAGPI Survey: radial trends in star formation across different cosmological simulations in comparison with observations at 0.3
Marcie Mun, Emily Wisnioski, Katherine E. Harborne +20
We investigate the internal and external mechanisms that regulate and quench star formation (SF) in galaxies at using MAGPI observations and the EAGLE, Magneticum, and…
The diverse star formation histories of early massive, quenched galaxies in modern galaxy formation simulations
Claudia del P. Lagos, Francesco Valentino, Ruby J. Wright +13
We present a comprehensive study of the star formation histories of massive-quenched galaxies at in 3 semi-analytic models (SHARK, GAEA, GALFORM) and 3 cosmological hydrodyna…
Quenching massive galaxies across cosmic time with the semi-analytic model SHARK v2.0
Claudia D. P. Lagos, Matias Bravo, Rodrigo Tobar +7
We introduce version 2.0 of the SHARK semi-analytic model of galaxy formation after many improvements to the physics included. The most significant being: (i) a model describing th…
GAMA/DEVILS: Cosmic star formation and AGN activity over 12.5 billion years
Jordan C. J. D'Silva, Simon P. Driver, Claudia D. P. Lagos +11
We use the Galaxy and Mass Assembly (GAMA) and the Deep Extragalactic Visible Legacy Survey (DEVILS) observational data sets to calculate the cosmic star formation rate (SFR) and a…
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…
KiDS-Legacy calibration: unifying shear and redshift calibration with the SKiLLS multi-band image simulations
Shun-Sheng Li, Konrad Kuijken, Henk Hoekstra +9
We present SKiLLS, a suite of multi-band image simulations for the weak lensing analysis of the complete Kilo-Degree Survey (KiDS), dubbed KiDS-Legacy analysis. The resulting catal…
Galaxy And Mass Assembly (GAMA): Data Release 4 and the z < 0.1 total and z < 0.08 morphological galaxy stellar mass functions
Simon P. Driver, Sabine Bellstedt, Aaron S. G. Robotham +67
In Galaxy And Mass Assembly Data Release 4 (GAMA DR4), we make available our full spectroscopic redshift sample. This includes 248682 galaxy spectra, and, in combination with earli…
Deep Extragalactic VIsible Legacy Survey (DEVILS): Identification of AGN through SED Fitting and the Evolution of the Bolometric AGN Luminosity Function
Jessica E. Thorne, Aaron S. G. Robotham, Luke J. M. Davies +15
Active galactic nuclei (AGN) are typically identified through radio, mid-infrared, or X-ray emission or through the presence of broad and/or narrow emission lines. AGN can also lea…
Deep Extragalactic VIsible Legacy Survey (DEVILS): Evolution of the -M relation and implications for self-regulated star formation
L. J. M. Davies, J. E. Thorne, S. Bellstedt +13
We present the evolution of the star-formation dispersion - stellar mass relation (-M) in the DEVILS D10 region using new measurements derived using the ProSpect…
Simultaneous Estimation of Large-Scale Structure and Milky Way Dust Extinction from Galaxy Surveys
Matías Bravo, Eric Gawiser, Nelson D. Padilla +3
The high cosmological precision offered by the next generation of galaxy surveys hinges on improved corrections for Galactic dust extinction. We explore the possibility of estimati…
Deep Extragalactic VIsible Legacy Survey (DEVILS): Consistent multi-wavelength photometry for the DEVILS regions (COSMOS, XMMLSS & ECDFS)
L. J. M. Davies, J. E. Thorne, A. S. G. Robotham +23
The Deep Extragalactic VIsible Legacy Survey (DEVILS) is an ongoing high-completeness, deep spectroscopic survey of 60,000 galaxies to Y21.2 mag, over 6 deg2 in thre…
Forensic reconstruction of galaxy colour evolution and population characterisation
Matías Bravo, Aaron S. G. Robotham, Claudia del P. Lagos +3
Mapping the evolution of galaxy colours, from blue star-forming to red passive systems, is fundamental to understand the processes involved in galaxy evolution. To this end, we rec…
Unveiling the atomic hydrogen-halo mass relation via spectral stacking
Garima Chauhan, Claudia del P. Lagos, Adam R. H. Stevens +5
Measuring the HI-halo mass scaling relation (HIHM) is fundamental to understanding the role of HI in galaxy formation and its connection to structure formation. While direct measur…
Deep Extragalactic VIsible Legacy Survey (DEVILS): SED Fitting in the D10-COSMOS Field and the Evolution of the Stellar Mass Function and SFR- relation
Jessica E. Thorne, Aaron. S. G. Robotham, Luke J. M. Davies +11
We present catalogues of stellar masses, star formation rates, and ancillary stellar population parameters for galaxies spanning from the Deep Extragalactic VIsible Legacy…
From rest-frame luminosity functions to observer-frame colour distributions: tackling the next challenge in cosmological simulations
Matías Bravo, Claudia del P. Lagos, Aaron S. G. Robotham +2
Galaxy spectral energy distributions (SEDs) remain among the most challenging yet informative quantities to reproduce in simulations due to the large and complex mixture of physica…
From the far-ultraviolet to the far-infrared -- galaxy emission at in the Shark semi-analytic model
Claudia del P. Lagos, Aaron S. G. Robotham, James W. Trayford +8
We combine the Shark semi-analytic model of galaxy formation with the ProSpect software tool for spectral energy distribution (SED) generation to study the multi-wavelength emissio…