A New Infrared Galaxy Count Model and Its Application to the AKARI Deep Field South

Details A New Infrared Galaxy Count Model and Its Application to the AKARI Deep Field South A New Infrared Galaxy Count Model and Its Application to the AKARI Deep Field South

Dec 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aspc..418..531t&link_type=abstract

AKARI, a Light to Illuminate the Misty Universe ASP Conference Series, Vol. 418, proceedings of a conference held 16-19 February

Astronomy and Astrophysics

Astronomy

Scientific paper

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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