  We present here the analysis performed using the pyPipe3D pipeline for the
final MaNGA dataset included in the SDSS seventeenth data-release. This dataset
comprises more than 10,000 individual datacubes, being the integral field
spectroscopy galaxy survey with the largest number of galaxies. pyPipe3D
processes the IFS datacubes to extract spatially-resolved spectroscopic
properties of both the stellar population and the ionized-gas emission lines. A
brief summary of the properties of the sample and the characteristics of the
analyzed data are included. The article provides details on (i) the performed
analysis, (ii) a description of the pipeline, (iii) the adopted stellar
population library, (iv) the morphological and photometric analysis, (v) the
adopted datamodel for the derived spatially resolved properties and (vi) the
individual integrated and characteristic galaxy properties included in a final
catalog. Comparisons with results from a previous version of the pipeline for
earlier data releases and from other tools using this dataset are included. A
practical example on how to use of the full dataset, and final catalog
illustrates how to handle the delivered product. Our full analysis can be
accessed and downloaded from the webpage
http://ifs.astroscu.unam.mx/MaNGA/Pipe3D_v3_1_1/.
