produced by standard <span style="font-variant:small-caps;">sas</span> tasks, to generate wavelet images and ends with a <span style="font-variant:small-caps;">sextractor</span> source list. <span style="font-variant:small-caps;">Xamin</span> characterises the sources with a maximum likelihood fit with both a pointlike and an extended ($\beta$-profile) model, and provides a <span style="font-variant:small-caps;">fits</span> file for each pointing with basic parameters separately for the soft \[0.5-2\] keV, or B, band and for the hard \[2-10\] keV, or CD, band.

The parameters produced by <span style="font-variant:small-caps;">Xamin</span> (which can be summarised as exposure times, statistics, raw source positions, source and background counts, and source count rates) are listed in detail in Table 1 of and Table 2 of @2006MNRAS.372..578P, and are flagged in Col. 4 (‘X’) of Tables \[TabBand\] and \[TabMerge\] of this paper. Other parameters are computed a posteriori during database ingestion on individual bands, as in @2013MNRAS.429.1652C. These parameters include the following:

-   The application of the C1/C2 recipe to classify extended sources [@2006MNRAS.372..578P], which are characterised by\
    the C1 recipe for a sample of clusters uncontaminated by point-like sources,\
       <span style="font-variant:small-caps;">ext $>$ 5and ext\_stat $>$ 33 and ext\_det\_stat $>$ 32</span>, and\
    the C2 recipe for clusters allowing a 50% contamination by misclassified point sources,\
       <span style="font-variant:small-caps;">ext $>$ 5and ext\_stat $>$ 15</span>;

    