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Updated: May 5, 2026

Characterizing Far-infrared Laser Emissions and the Measurement of Their Frequencies
Published on: December 18, 2015
Over half of the far-infrared background light comes from galaxies at z >or= 1.2
Mark J Devlin1, Peter A R Ade, Itziar Aretxaga
1Department of Physics & Astronomy, University of Pennsylvania, 209 South 33rd Street, Philadelphia, Pennsylvania 19104, USA. devlin@physics.upenn.edu
Abstract:
Submillimetre surveys during the past decade have discovered a population of luminous, high-redshift, dusty starburst galaxies. In the redshift range 1
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