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Infrared molecular hydrogen lines in GRB host galaxies

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Figure

Figure 1. The LIRIS spectrum of the host galaxy of GRB 080517.γFor plotting purposes the spectrum is smoothed with a 3 pixel me-dian filter
Figure 3. X-Shooter spectrum of the host galaxy of GRB 031203,around the location of the H2 1–0 S(3) transition, whose wave-length at the host redshift is marked with a dashed red line; thewavelength is as observed
Figure 4. A small section of the Spitzer spectrum with the PAH-FIT fit is shown (note that the model is fit over the full Spitzerrange, see Section 4.1)
Table 2.Listed are the flux ratios of the molecular line fluxes (or limits) divided by the Paschen α line flux

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