Determining star formation rates of active galactic nuclei host galaxies
  based on SED fitting with sub-mm data
  We present the star formation rate (SFR) measurements based on the spectral
energy distribution (SED) analysis with new sub-mm fluxes combined with
archival 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 the
James Clerk Maxwell Telescope, and obtained flux or an upper limit at 450 and
850 $\mu$m for each target. By experimenting the effect of the AGN dust
component in the SED fit, we find that dust luminosity can be overestimated if
AGN contribution is ignored. While the SFR based on 4000{\AA} break shows a
significant offset compared to dust luminosity based SFR, the SFR obtained by
the artificial neural network (Ellison et al. 2016) generally shows consistency
albeit with a large scatter. We find that SFR correlates with AGN outflow
strength manifested by the [OIII] $\lambda 5007$ emission line, and that AGNs
with higher Eddington ratios and stronger outflows are in general hosted by
galaxies with higher SFR, which is consistent with the correlation reported by
Woo et al. (2020). This suggests no instantaneous quenching of star formation
due to AGN feedback.
