Fig. 7
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X-ray luminosity as function of specific radio luminosity for the SMGPS-RASS (left) and eRASS1 (right) sources. In each panel, the solid line shows the fit to that dataset, while the dashed line shows the fit obtained from the other dataset. The markers show object/spectral-type information obtained from either SIMBAD or Gaia Collaboration (2023) Gaia DR3 astrophysical parameters.
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