SEDs and best fit spectra of two galaxies, one with a good  and one with a worse fit. Points are photometric points, from broad-band photometry (brown) and from the grism spectra (red). Error bars in the wavelength direction show the FWHM of the filter with which the point was observed. The grey spectrum is the best fit spectrum from the models, with green, yellow and blue lines showing the spectra convolved with the resolution profile for each galaxy for the 1 SSP, 2 SSP and constant SFR scenarios. LBG_46190 (left) has a  whereas LBG_53929 has a  (right). The brightest of the grism data points in the LBG_53929 SED is due to a strong [OII] emission line.