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Table 1: Comparison of the extragalactic and asteroid full fluctuation power levels at some representative wavelengths of infrared and submillimetre space instruments. Asteroid fluctuation power was derived at the specified $\lambda$ - $\lambda _{\odot }$ helioecliptic longitude, and at the ecliptic plane. The columns of the table are: 1) name of the instrument; 2) wavelength; 3) extragalactic background fluctuation power (EGB); 4) asteroid fluctuation power (MBA); 5) solar elongation used in the MBA fluctuation power calibration, in accordance with the visibility constraints of the instrument; 6) Ecliptic latitude range above/below the ecliptic plane, where a specific instrument is considered as "affected'' by asteroid confusion noise. Missing values indicate that the instrument is not affected.