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Fig. 12.
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Infrared star formation rate (SFR) distribution for the RDQs and RUQs derived from the infrared luminosity LIR with ≥2σ SPIRE-250 μm detections. The mean SFR of the samples are indicated by the dashed lines. The mean SFRs of our quasar samples are consistent with those of the main sequence star-forming galaxies.
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