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P185
The formation of submillimetre-bright galaxies from gas infall over a billion years.Kinematic classifications of local interacting galaxies: implications for the merger/disk classifications at high-zALMA Resolves the Nuclear Disks of Arp 220ALMA imaging of HCN, CS, and dust in Arp 220 and NGC 6240Rotation curve fitting and its fatal attraction to cores in realistically simulated galaxy observationsSynthetic galaxy images and spectra from the Illustris simulationThe star formation main sequence and stellar mass assembly of galaxies in the Illustris simulationGalaxy mergers on a moving mesh: a comparison with smoothed particle hydrodynamicsThe AGN luminosity fraction in merging galaxiesFast molecular outflow from a dusty star-forming galaxy in the early UniverseWhat FIREs up star formation: the emergence of the Kennicutt–Schmidt law from feedbackSimulating galaxies in the reionization era with FIRE-2: galaxy scaling relations, stellar mass functions, and luminosity functionsDiscrete Effects in Stellar Feedback: Individual Supernovae, Hypernovae, and IMF Sampling in Dwarf GalaxiesSubmillimetre flux as a probe of molecular ISM mass in high-z galaxiesFIRE-2 simulations: physics versus numerics in galaxy formationSimulating galaxies in the reionization era with FIRE-2: morphologies and sizesObservational constraints on the physical nature of submillimetre source multiplicity: chance projections are commonPanchromatic SED modelling of spatially resolved galaxiesHow to model supernovae in simulations of star and galaxy formationFormation of globular cluster candidates in merging proto-galaxies at high redshift: a view from the FIRE cosmological simulationsStellar feedback strongly alters the amplification and morphology of galactic magnetic fieldsIs a top-heavy initial mass function needed to reproduce the submillimetre galaxy number counts?SIDM on FIRE: hydrodynamical self-interacting dark matter simulations of low-mass dwarf galaxies.Stacked Star Formation Rate Profiles of Bursty Galaxies Exhibit “Coherent” Star FormationFeedback first: the surprisingly weak effects of magnetic fields, viscosity, conduction and metal diffusion on sub-L* galaxy formationA Controlled Study of Cold Dust Content in Galaxies from z = 0–2The IRX–βRelation: Insights from SimulationsHow stellar feedback simultaneously regulates star formation and drives outflowsThe role of star formation and AGN in dust heating of z=0.3-2.8 galaxies - II. Informing IR AGN fraction estimates through simulationsWhere stars form: inside-out growth and coherent star formation from HST H{alpha} maps of 3200 galaxies across the main sequence at 0.7 < z < 1.5What shapes the far-infrared spectral energy distributions of galaxies?Merger signatures in the dynamics of star-forming gasVariations of the ISM compactness across the main sequence of star forming galaxies: observations and simulationsDeriving star formation histories from photometry using energy balance spectral energy distribution modellingThe bias of the submillimetre galaxy population: SMGs are poor tracers of the most-massive structures in thez ∼ 2 UniverseThe total infrared luminosity may significantly overestimate the star formation rate of quenching and recently quenched galaxiesDetermining the stellar masses of submillimetre galaxies: the critical importance of star formation historiesShould we believe the results of ultraviolet–millimetre galaxy spectral energy distribution modelling?Simulated galaxy interactions as probes of merger spectral energy distributionsModeling mid-infrared diagnostics of obscured quasars and starbursts
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description
researcher ORCID ID = 0000-0003-4073-3236
@en
wetenschapper
@nl
name
Christopher Hayward
@ast
Christopher Hayward
@en
Christopher Hayward
@es
Christopher Hayward
@nl
type
label
Christopher Hayward
@ast
Christopher Hayward
@en
Christopher Hayward
@es
Christopher Hayward
@nl
prefLabel
Christopher Hayward
@ast
Christopher Hayward
@en
Christopher Hayward
@es
Christopher Hayward
@nl
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0000-0003-4073-3236