Fig. 1.
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Bolometric luminosity as a function of redshift. The grey contours highlight the AGNs of Yamada et al. (2024a, Y24), the red ones are the data from Laor & Behar (2008, LB08), and those in purple the data from Panessa & Giroletti (2013, PG13). We choose LB08 and PG13 as a comparison for the study of the X-ray-radio luminosity correlation. Then we plot the objects in the SUBWAYS sample (blue empty dots) and a comparison sample from Tombesi et al. (2010, T10, black empty diamonds). UFO hosts are marked by stars and triangles in SUBWAYS and T10 respectively.
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