| Issue |
A&A
Volume 537, January 2012
|
|
|---|---|---|
| Article Number | A15 | |
| Number of page(s) | 19 | |
| Section | Extragalactic astronomy | |
| DOI | https://doi.org/10.1051/0004-6361/201117414 | |
| Published online | 20 December 2011 | |
Online material
Appendix A: SED fits
 |
Fig. A.1
NIR through to X-ray SEDs of the 17 GRBs in our final sample with the best-fit FM90 model overplotted. Frequency is plotted in the rest-frame and flux density is in arbitrary units for clarity. The SEDs have been corrected for Galactic reddening and soft X-ray absorption, and both the host galaxy absorbed/extinguished (solid) and intrinsic (dashed) best-fit afterglow SED are indicated. The afterglow SEDs are ordered by afterglow host galaxy extinction, with the most extinguished at the bottom, and the least at the top. |
| Open with DEXTER | |
 |
Fig. A.2
NIR through to X-ray SEDs of the 32 GRBs analysed that did not enter our final sample. Frequency is plotted in the rest-frame and flux density is in arbitrary units for clarity. The SEDs have been corrected for Galactic reddening and soft X-ray absorption, and both the host galaxy absorbed/extinguished (solid) and intrinsic (dashed) best-fit afterglow SED are indicated. The afterglow SEDs are ordered by afterglow host galaxy extinction, with the most extinguished at the bottom, and the least at the top. |
| Open with DEXTER | |
 |
Fig. A.2
continued. |
| Open with DEXTER | |
 |
Fig. A.2
continued. |
| Open with DEXTER | |
© ESO, 2012
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