Changing-look Seyfert galaxies with optical linear polarization measurements

In this lecture note, we make the case for new (spectro)polarimetric measurements of ``changing-look'' AGNs (CLAGNs), a subclass of the AGN family tree that shows long-term (months to years) large flux variability associated with the appearance or disappearance of optical broad emission lines. We discuss how polarization measurements could help to distinguish which of the several scenarios proposed to explain such variations is/are the most likely. We collected all the past polarization measurements of nearby, Seyfert-like CLAGNs and take stock that almost all polarimetric information we have on those fascinating objects dates from the 80's and 90's. We thus explain how polarization could help us understanding the physical processes happening in the first parsecs of CLAGNs and why new polarization monitoring campaigns are strongly needed.