Notes. The first columns contains the source id of the star followed, in columns two and three, by the apparent G magnitude and the BP-RP colour. Then, columns four to nine contain, respectively, the right ascension, declination, proper motion in both, and their uncertainties. Then, on the tenth and eleventh columns we include the period-Wesenheit distances and their uncertainties for our sub-sample of RR Lyrae. Columns 12 and 13 correspond, respectively, to the value of radial velocity adopted and the catalogues used to obtain it (A - APOGEE, L - LAMOST, S - SEGUE, G - Gaia, C - SIMBAD). Then, on column 14, we show the [α/M] abundance from APOGEE. The next six columns show the metallicities from APOGEE, LAMOST and SEGUE, in that order, followed by their respective signal-to-noise ratios (for APOGEE, we used SNREV). Finally, the last four columns carry the different probabilities that we have calculated: probability of a star of belonging to the bright branch (col. 21), of belonging to the faint (col. 22), of belonging to the Sgr stream (col. 23) and the parallax_over_error score (col. 24). The full table is available at CDS.