| Abstract |
Far-infrared galaxies, which are luminous in far-infrared emitted by dust grains, are good tracers of star forming activity in the Universe. The power spectrum, represented as a function of squared Fourier coefficients F(k), is the statistical quantity to measure of the inhomogeneity of galaxy distribution in the Universe. With the power spectrum of the far-infrared galaxy distribution, we can see the properties of the distribution of star forming galaxies. In our study, we use the AKARI / FIS all sky survey data and calculate the power spectrum. In this talk, we compare our result to the previous study and discuss the properties of the infrared galaxies detected by AKARI. |
