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30 papers
Identification of two bright z>3 submillimeter galaxy candidates in the COSMOS field
M. Aravena, J. D. Younger, G. G. Fazio +5
We present high-resolution interferometric Submillimeter Array (SMA) imaging at 890 microns (~2" resolution) of two millimeter selected galaxies -- MMJ100015+021549 and MMJ100047+0…
Mergers in Lambda-CDM: Uncertainties in Theoretical Predictions and Interpretations of the Merger Rate
Philip F. Hopkins, Darren Croton, Kevin Bundy +10
Different methodologies lead to order-of-magnitude variations in predicted galaxy merger rates. We examine and quantify the dominant uncertainties. Different halo merger rates and…
Deep, ultra-high-resolution radio imaging of submillimetre galaxies using Very Long Baseline Interferometry
A. D. Biggs, J. D. Younger, R. J. Ivison
We present continent-scale VLBI - obtained with the European VLBI Network (EVN) at a wavelength of 18cm - of six distant, luminous submm-selected galaxies (SMGs). Our images have a…
A physical model for the origin of the diffuse cosmic infrared background
Joshua D. Younger, Philip F. Hopkins
We present a physical model for origin of the cosmic diffuse infrared background (CDIRB). By utilizing the observed stellar mass function and its evolution as input to a semi-empir…
The physical scale of the far-infrared emission in the most luminous submillimetre galaxies II: evidence for merger-driven star formation
J. D. Younger, G. G. Fazio, M. L. N. Ashby +11
We present high-resolution 345 GHz interferometric observations of two extreme luminous (L_{IR}>10^{13} L_sun), submillimetre-selected galaxies (SMGs) in the COSMOS field with the…
Intense Star Formation within Resolved Compact Regions in a Galaxy at z=2.3
Mark Swinbank, Ian Smail, Steve Longmore +18
Massive galaxies in the early Universe have been shown to be forming stars at surprisingly high rates. Prominent examples are dust-obscured galaxies which are luminous when observe…