Analysis flow for the PHANGS-MUSE DAP. After spectral re-binning using a ln(λ) prescription, the resulting mosaicked cubes are used for the extraction of the stellar kinematics, stellar extinction, and stellar population maps, using an appropriate adaptive binning scheme, while the emission line maps (including the corresponding gas kinematics) are derived from the originally sampled cubes. The main information pertaining to the stellar libraries, spectral masks, assumptions and fixed input for each step are mentioned in the upper part of the figure, while the data products are illustrated in its lower part. See Sect. 5.2 for further details.