Relationship between the [O II]3727 equivalent width and the derived stellar mass for our emitters (cyan open circles). The black diamonds are the median of our emitters for bins 0.5 dex in log(M_*/M_⊙), and the data from Paulino-Afonso et al. (2020) (red closed squares), Darvish et al. (2015) (filled purple stars for filament galaxies and green triangles for field galaxies), and Reddy et al. (2018) (grey diamonds). The black dashed line represents the best fit for all the binned data and the cyan point-dashed line represent the best fit for the only the binned data of the emitters detected in this work. The pink band represents the power law fit with uncertainties from Khostovan et al. (2016) for [O II]3727 emitters at z = 1.47.