Galaxy and AGN counts model

Angular power spectra
100 μm:
100 micron angular power spectrum


160 μm:
160 micron angular power spectrum


250 μm by sources with S < 50 mJy:
250 micron angular power spectrum for souce with flux density smaller than 50 mJy


350 μm by sources with S < 50 mJy:
350 micron angular power spectrum for souce with flux density smaller than 50 mJy


500 μm by sources with S < 50 mJy:
500 micron angular power spectrum for souce with flux density smaller than 50 mJy



Cross-correlations at submm wavelengths
250 μm X 350 μm:
250 and 350 micron cross-frequency power spectra


250 μm X 500 μm:
250 and 500 micron cross-frequency power spectra


350 μm X 500 μm:
350 and 500 micron cross-frequency power spectra