Fig. 5.

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Relation between SFR and M* for existing MaNGA AGN catalogs. The gray-colored image represents the density of MaNGA galaxies in the plot. The RDAGN studied in this work are indicated in green. Dark yellow contours represent the density of AGN host galaxies for from the Comerford et al. (2020) AGN catalog, the dark blue contours represent the density of galaxies from the Sánchez et al. (2018) AGN catalog, the Wylezalek et al. (2018) AGN catalog are represented by orange contours, and the red contours exhibit the density of Rembold et al. (2017) AGN catalog. The SFR–M* space is divided into 50 × 50 bins, and the contours are drawn at 25, 50, 75, and 100% of the maximum number density. The dotted line represents the SFMS derived for SDSS-IV MaNGA galaxies derived by Cano-Díaz et al. (2019), the dark gray shading represents the errors on slope, and the light gray shading represents the standard deviation.
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