NICER observation list: Target ID 753801

The drastic changes seen in changing look AGNs (CL-AGNs) in short timescales (a few months to years) are challenging the simplest form of the AGN unification framework which predicts that such changes occur over far longer timescales. It seems likely that CL-AGN events are driven by surprisingly rapid and extreme changes in the accretion disk around the supermassive black hole (SMBH), which also affects the coronal emission causing large unexplained variations in flux and spectral states. The CL-AGN are therefore ideal test beds to understand the properties of coronal X-ray emission. We propose a ToO campaign targeting a newly discovered CL-AGN meeting our criteria in the upcoming cycle. Once triggered, we propose biweekly NICER monitoring, 2 ks per visit, for 6 months (total 96 ks).