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Over half of the far-infrared background light comes from galaxies at z >= 1.2
Mark J. Devlin, Peter A. R. Ade, Itziar Aretxaga +26
Submillimetre surveys during the past decade have discovered a population of luminous, high-redshift, dusty starburst galaxies. In the redshift range 1 <= z <= 4, these massive sub…
Radio and mid-infrared identification of BLAST source counterparts in the Chandra Deep Field South
Simon Dye, Peter A. R. Ade, James J. Bock +28
We have identified radio and/or mid-infrared counterparts to 198 out of 350 sources detected at >=5 sigma over ~ 9 square degrees centered on the Chandra Deep Field South (CDFS) by…
A Bright Submillimeter Source in the Bullet Cluster (1E0657--56) Field Detected with BLAST
Marie Rex, Peter A. R. Ade, Itziar Aretxaga +26
We present the 250, 350, and 500 micron detection of bright submillimeter emission in the direction of the Bullet Cluster measured by the Balloon-borne Large Aperture Submillimeter…
Observing the Evolution of the Universe
James Aguirre, Alexandre Amblard, Amjad Ashoorioon +172
How did the universe evolve? The fine angular scale (l>1000) temperature and polarization anisotropies in the CMB are a Rosetta stone for understanding the evolution of the univers…
The Origin of the Universe as Revealed Through the Polarization of the Cosmic Microwave Background
S. Dodelson, R. Easther, S. Hanany +61
Modern cosmology has sharpened questions posed for millennia about the origin of our cosmic habitat. The age-old questions have been transformed into two pressing issues primed for…