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We present the star formation rate (SFR) measurements based on the spectralenergy distribution (SED) analysis with new sub-mm fluxes combined witharchival multi-wavelength data for a sample of 52 AGN host galaxies at z$<0.2$. We carried out sub-mm observations using the SCUBA-2 camera at theJames Clerk Maxwell Telescope, and obtained flux or an upper limit at 450 and850 $\mu$m for each target. By experimenting the effect of the AGN dustcomponent in the SED fit, we find that dust luminosity can be overestimated ifAGN contribution is ignored. While the SFR based on 4000{\AA} break shows asignificant offset compared to dust luminosity based SFR, the SFR obtained bythe artificial neural network (Ellison et al. 2016) generally shows consistencyalbeit with a large scatter. We find that SFR correlates with AGN outflowstrength manifested by the [OIII] $\lambda 5007$ emission line, and that AGNswith higher Eddington ratios and stronger outflows are in general hosted bygalaxies with higher SFR, which is consistent with the correlation reported byWoo et al. (2020). This suggests no instantaneous quenching of star formationdue to AGN feedback.

Determining star formation rates of active galactic nuclei host galaxies based on SED fitting with sub-mm data