The X-ray statistical properties of dust-obscured galaxies detected by eROSITA

Open Access

Fig. 4.

L_6 μm estimated by CIGALE ( $L_{6 μ m}^{CIGALE}$ $L_{{6\,{\upmu}\mathrm{m}}}^{\mathrm{CIGALE}}$ ) versus the rest-frame 6 μm luminosity (L_6 μm) interpolated from the nearby WISE W1, W2, and W3 bands ( $L_{6 μ m}^{MIR}$ $L_{{6\,{\upmu}\mathrm{m}}}^{\mathrm{MIR}}$ ). Red stars represent the eFEDS-DOGs, while blue squares indicate the eFEDS-DOGs with BluDOG-like features. The solid black line corresponds to log L^MIR6 μm = log L^CIGALE6 μm.

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