Fig. 3
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Top: distribution of sources in the W1 band vs. soft X-ray flux parameter space for the ALLWISE counterparts to 2RXS (pink) and XMMSL2 (blue). The confirmed SPIDERS AGN are represented in yellow. The cut defined in Eq. (2) is also shown. W1–W2 magnitude plotted against the W2–W3 (middle) and W3–W4 (bottom). The black lines show the cuts applied based on the SPIDERS AGN position.
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