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The nature of the bright submillimeter galaxy population: a radio pre-selected sample with I>25
S. C. Chapman, E. Richards, G. Lewis +2
Deep submillimetre surveys have successfully detected distant, star-forming galaxies, enshrouded in vast quantities of dust and which emit most of their energy at far infrared wave…
The Nature of the Hard X-ray Background Sources: Optical, Near-infrared, Submillimeter, and Radio Properties
A. J. Barger, L. L. Cowie, R. F. Mushotzky +1
With recent Chandra observations, at least 60% of the 2-10 keV background is now resolved into discrete sources. Here we present deep optical, NIR, submm, and 20 cm (radio) images,…
Resolving the extragalactic hard X-ray background
R. F. Mushotzky, L. L. Cowie, A. J. Barger +1
The origin of the hard (2-10 keV) X-ray background has remained mysterious for over 35 years. Most of the soft (0.5-2 keV) X-ray background has been resolved into discrete sources,…
Mapping the Evolution of High Redshift Dusty Galaxies with Submillimeter Observations of a Radio-Selected Sample
A. J. Barger, L. L. Cowie, E. A. Richards
Direct submm imaging has recently revealed the 850-micron background to be mostly composed of a population of distant ultraluminous infrared galaxies, but identifying the optical/N…