LePHARE fit to the magnitudes of the GRB 111209A host galaxy. The detections are , the upper limits JJ_GH_GK_S,G (the subscript G denotes GROND filters presented in this work, the non-GROND data have been taken from L14). The red · marks represent the photometry values as determined by the synthetic SED. The fit is acceptable, χ² = 1.36. The host galaxy is very typical for a GRB host, a low-mass, low-extinction, young star-forming galaxy (see, e.g. Schulze et al. 2014 for a comparison). For specific values, see Table 6.