Point spread function reconstruction for SOUL + LUCI LBT data

Here, we present the status of an ongoing project aimed at developing a point spread function (PSF) reconstruction software for adaptive optics (AO) observations. In particular, test first time implementation pyramid wave-front sensor data on our algorithms. As step in assessing its reliability, applied to bright, on-axis, point-like sources using two independent sets observations, acquired with single-conjugated AO upgrade Large Binocular Telescope. Using only telemetry data, reconstructed PSF by carefully calibrating instrument response. The accuracy results has been evaluated classical metric: specifically, PSFs differ from observed ones <2 % Strehl ratio and 4.5% full-width half maximum. Moreover, recovered encircled energy associated core is accurate 4% level worst case. then considering idealized scientific test-case consisting measurements morphological parameters compact galaxy. future, will include analysis anisoplanatism, low signal-to-noise regimes, application multi-conjugated