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- Lawrence Berkeley National LaboratoryUS192 papers
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17 papers · 2 filters
Super-luminous supernovae at redshifts of 2.05 and 3.90
Jeff Cooke, Mark Sullivan, Avishay Gal-Yam +6
A rare class of `super-luminous' supernovae that are about ten or more times more luminous at their peaks than other types of luminous supernovae has recently been found at low to…
Cosmological origin of anomalous radio background
James M. Cline, Aaron C. Vincent
The ARCADE 2 collaboration has reported a significant excess in the isotropic radio background, whose homogeneity cannot be reconciled with clustered sources. This suggests a cosmo…
An ALMA survey of submillimetre galaxies in the Extended Chandra Deep Field South: High resolution 870um source counts
Alexander Karim, Mark Swinbank, Jackie Hodge +20
We report the first counts of faint submillimetre galaxies (SMG) in the 870-um band derived from arcsecond resolution observations with the Atacama Large Millimeter Array (ALMA). W…
The Properties of the Star-Forming Interstellar Medium at z=0.84-2.23 from HiZELS - I: Mapping the Internal Dynamics and Metallicity Gradients in High-Redshift Disk Galaxies
Mark Swinbank, David Sobral, Ian Smail +5
We present adaptive optics assisted, spatially resolved spectroscopy of a sample of nine H-alpha-selected galaxies at z=0.84--2.23 drawn from the HiZELS narrow-band survey. These g…
An ALMA survey of Sub-millimetre Galaxies in the Extended Chandra Deep Field South: Detection of [C II] at z=4.4
Mark Swinbank, Alexander Karim, Ian Smail +19
We present ALMA 870-um (345GHz) observations of two sub-millimetre galaxies (SMGs) drawn from an ALMA study of the 126 sub-millimeter sources from the LABOCA Extended Chandra Deep…
The Properties of the Star-Forming Interstellar Medium at z=0.8-2.2 from HiZELS - II: Star-Formation and Clump Scaling Laws in Gas Rich, Turbulent Disks
Mark Swinbank, Ian Smail, David Sobral +3
We present adaptive optics assisted integral field spectroscopy of nine Halpha-selected galaxies at z=0.84--2.23 selected from the HiZELS narrow-band survey. Our observations map t…