NICER observation list: Target ID 465201

We request 40 ks of NICER and 60 ks of NuSTAR time to trigger ToO observations to obtain high signal-to-noise spectra from the relatively under-explored fading phases of a non-failed outburst of transient black hole. Our principal goal is to track the evolving properties of the accretion-corona system viz., inner disk truncation, disk density, coronal geometry, and disk inclination as the outburst enters the returning hard-intermediate to quiescent-hard state. This will be achieved with a suite of relativistic reflection and reverberation models to investigate the implications of accretion physics on the origin of hysteresis in the hardness-intensity diagram.