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Paper: A New Infrared Galaxy Count Model and Its Application to the AKARI Deep Field South
Volume: 418, AKARI, a Light to Illuminate the Misty Universe
Page: 531
Authors: Takeuchi, T. T.; Ishii, T. T.
Abstract: Using the observed evolution of the far-IR (FIR) luminosity function (LF) of galaxies obtained with Spitzer, We improved the previous model under the strong constraint of the LF evolution. This model succeeded in reproducing many available FIR and submillimeter (submm) observations of galaxies and the cosmic IR background (CIB).
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