Example of a simulated spectrum from MAMBO of a galaxy at redshift z ∼ 1.6, stellar mass of log₁₀(M_*/M_⊙) = 10.8, H_E ∼ 21.1, SFR of 232.7 M_⊙/yr, effective disk radius of $0\stackrel{″}{.}66$, and a B/T of 0.33. The black spectrum represents the incident model spectrum at its native resolution (∼0.27 nm). The EWS simulated spectrum is shown in grey, whilst the blue and red spectra correspond to the EDS blue and red grism simulated observations, respectively. The top panel focuses on the stellar continuum, whilst the bottom panels highlights key emission lines spectral regions: note how the increased survey depth of the EDS allows for the detection of fainter emission lines, such as [O III]λ4959.