Abstract
The angular distribution of the IRAS galaxies has been expanded in spherical harmonics and its angular power spectrum has been calculated. This distribution is dominated by the first few multipoles and the amplitude is a decreasing function of l. We find the IRAS data to have more power on the scale of a few x 10h — 1Mpc compared with the standard CDM model, and to be compatible with an open universe CDM model of Ω0 h = 0.2.
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