This work utilizes the photometric data from two DECam programs, 2016A-0618 and 2017B-0906, focusing on the region between the MCs. On 2018 February 12-13, we used M2FS, a multi-object fiber spectrograph at the Magellan Clay 6.5m telescope, to acquire spectra for the selected targets. Table 2 presents spectroscopic parameter measurements for all the stars that either have S/N larger than 3 or have RV uncertainty less than 10km/s. We list measurements of the effective temperature, surface gravity, metallicity, and heliocentric LOS velocity. We also provide in the table, the g, r magnitudes and the log odds of being Hydrus 1 member star, based on the model described in the next section.