SIMBAD references

Line flux ratios from [O II] doublets can probe electron densities in the interstellar medium of galaxies. We employ the Southern African Large Telescope's (SALT) Robert Stobie Spectrograph (RSS), which provides sufficient resolution (R ∼ 3000) to split the [O II] doublets, to target galaxies from Hobby-Eberly Telescope Dark Energy Experiment and One-hundred-deg² DECam Imaging in Narrowbands with emission line fluxes of at least 2 × 10^–16 erg cm^–2 s^–1. Reduction is carried out using RSSMOSPipeline to reduce SALT-RSS data through wavelength calibration. Despite SALT-RSS being known for its difficulty to flux calibrate, we present spectra that have been flux calibrated using alignment stars with Sloan Digital Sky Survey spectra as standards. We combine multiple spectroscopic settings to obtain full 2D spectra across a wavelength range of 3500-9500 Å. A 1D spectrum can then be extracted to calculate flux ratios and line widths, revealing important physical properties of these bright [O II]-emitters.