VST/OmegaCAM u,g,r,i,Ha light curves for YSOs in the Lagoon Nebula

Collection of VST/OmegaCAM light curve files for all young stellar objects in the Lagoon Nebula region that have been identified as members or candidate members in Table 1 of Venuti et al. (2024, AJ, 167, 120). These photometric time series were obtained in 2016 (program id 297.C-5033(A)), reduced as described in Venuti et al. (2021, AJ, 162, 101), and analyzed in Venuti et al. (2024). Individual sources are matched to the corresponding datafiles by their identifier, as listed in the first column of Table 1 in Venuti et al. (2024) and in the datafile name. Each datafile, in .txt format, contains four columns: Modified Julian Date, magnitude, magnitude uncertainty, and filter (u/g/r/i/Ha). All magnitudes have been calibrated to the VPHAS+ survey catalog (Drew et al. 2014, MNRAS, 440, 2036).