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Fig. A.2.

image

SED of the host galaxy of GRB 071112C (corrected for Galactic extinction) based on GROND gri′-band data, a GTC z′, an HST/F160W (H band), and a Spitzer/IRAC1 detection as well as data taken with Keck/LRIS and Gemini-N/GMOS (Table C.11). In JKs we have only GROND upper limits (Table C.6). The solid line displays the best template fit using Le PHARE, green data points are the template-predicted magnitudes. Potential host-galaxy emission lines are indicated.

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