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JAXA Repository AIREX: MIDINFRARED VARIABILITY OF ACTIVE GALACTIC NUCLEI WITH THE AKARI AND WISE ALLSKY SURVEYS

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TABLE 1 Continued.
Fig. 1.— Distribution of the variability criteria, S defined in Equation 5. The abscissa shows S of each source, and the ordinate the number of sources
Fig. 2.— Frequency distribution of the relative flux variations for the total sample of AGN in the S9W-W3 band (left panel) and L18W-W4 band (right panel)
Fig. 3.— Signal-to-Noise (S/N) ratio, defined as the AKARI flux divided by its error, of A- and F-type stars detected by both AKARI and WISE are plotted against the AKARI fluxes
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