Dependency of the OA, UGC, QSOC, and TGE modules on the DSC combined probabilities for the selection of the sources to be processed (classprob_dsc_combod, see Sect. 3 for a definition). For each module, we provide a synthetic view of their input and output, and the number of sources for which the module produces results in Gaia DR3. In the case of TGE, we provide the number of extinction estimates that were computed in level 9 HEALPixes (see Sect. 7). Unlike the other modules described here, TGE additionally relies on the General Stellar Parametrizer from Photometry (GSP-Phot) for its source selection and processing, which is described in Andrae et al. (2022).