Understanding infrared (IR) luminosity is fundamental to understanding the cosmic star formation history and AGN evolution, since their most intense stages are often obscured by dust. Japanese infrared satellite, AKARI, provided unique data sets to probe this both at low and high redshifts. The AKARI performed an all sky survey in 6 IR bands (9, 18, 65, 90, 140, and 160μm ) with 3-10 times better sensitivity than IRAS, covering the crucial far-IR wavelengths across the peak of the dust emission. Combined with a better spatial resolution, AKARI can measure the total infrared luminosity ( LTIR) of individual galaxies much more precisely, and thus, the total infrared luminosity density of the local Universe. In the AKARI NEP deep field, we construct restframe 8μm, 12μm , and total infrared (TIR) luminosity functions (LFs) at 0.15 < z < 2.2 using 4,128 infrared sources. A continuous filter coverage in the mid-IR wavelength (2.4, 3.2, 4.1, 7, 9, 11, 15, 18, and 24μm ) by the AKARI satellite allows us to estimate restframe 8μm and 12μm luminosities without using a large extrapolation based on a SED fit, which was the largest uncertainty in previous work. By combining these two results, we reveal dust-hidden cosmic star formation history and AGN evolution from z = 0 to z = 2.2, all probed by the AKARI satellite.

ABSTRACT
1. INTRODUCTION
2. AKARI ALL SKY SURVEY: LOW-z UNIVERSE
3. AKARI NEP DEEP FIELD: HIGH-z UNIVERSE
    3.1. 8 μm LF
    3.2. 12 μm LF
    3.3. TIR LF
4. COSMIC STAR FORMATION HISTORY
5. COSMIC AGN ACCREATION HISTORY
REFERENCES

• TOMOTSUGU GOTO(Dark Cosmology Centre, Niels Bohr Institute, University of Copenhagen)
• AKARI NEP TEAM(Dark Cosmology Centre, Niels Bohr Institute, University of Copenhagen)
• AKARI ALL SKY SURVEY TEAM(Dark Cosmology Centre, Niels Bohr Institute, University of Copenhagen)