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Fig. 3
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BlaST-derived synchrotron peak frequency as a function of the 0.2–12 keV/1.4 GHz flux ratio (left) and of the 0.2–12 keV flux (right) for the 1007 5BZCAT sources without a Fermi-LAT counterpart and with an X-ray counterpart. The sources are color-coded according to class using the same coding as that described in Figure 2.
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