  We introduce our project, AGNSTRONG (Active Galactic Nuclei and STaR
fOrmation in Nearby Galaxies). Our research goals encompass investigating the
kinematic properties of ionized and molecular gas outflows, understanding the
impact of AGN feedback, and exploring the coevolution dynamics between AGN
strength activity and star formation activity. We aim to conduct a thorough
analysis to determine whether there is an increase or suppression in SFRs among
targets with and without powerful relativistic jets. Our sample consists of 35
nearby AGNs with and without powerful relativistic jet detections. Utilizing
sub-millimeter (sub-mm) continuum observations at 450 {\mu}m and 850 {\mu}m
from SCUBA-2 at the James Clerk Maxwell Telescope, we determine star-formation
rates (SFRs) for our sources using spectral energy distribution (SED) fitting
models. Additionally, we employ high-quality, spatially resolved spectra from
UV-optical to near-infrared bands obtained with the Double Spectrograph and
Triple Spectrograph mounted on the 200-inch Hale telescope at Palomar
Observatory to study their multiphase gas outflow properties. This paper
presents an overview of our sample selection methodology, research strategy,
and initial results of our project. We find that the SFRs determined without
including the sub-mm data in the SED fitting are overestimated by approximately
0.08 dex compared to those estimated with the inclusion of sub-mm data.
Additionally, we compare the estimated SFRs in our work with those traced by
the 4000{\AA} break, as provided by the MPA-JHU catalog. We find that our
determined SFRs are systematically higher than those traced by the 4000{\AA}
break. Finally, we outline our future research plans.
