Spectral energy distribution of the host galaxy. We have obtained thorough multi-band photometry of this host as part of the SHOALS survey, showing it to be a remarkably luminous (MUV ~ –23 mag) Lyman-break galaxy. A notable excess in the K_s-band photometry above the SED model suggests very strong high equivalent-width [OIII] emission. Clear circles show bands not used in the SED fit due to Ly-α forest or nebular contamination. Empty squares represent the value of the model integrated over the width of each band, and they show a relatively good fit.