| Issue |
A&A
Volume 577, May 2015
|
|
|---|---|---|
| Article Number | A44 | |
| Number of page(s) | 15 | |
| Section | Extragalactic astronomy | |
| DOI | https://doi.org/10.1051/0004-6361/201321936 | |
| Published online | 29 April 2015 | |
Online material
Appendix A: Optical/NIR photometry
The three tables presented as follows are corrected for Galactic foreground extinction (Schlegel et al. 1998).
GRB 081007/SN 2008hw.
GRB 091127/SN 2009nz.
GRB 101219B/SN 2010ma.
Appendix B: Sequences of standard stars
The sequence of reference stars in the field of GRB 091127/SN 2009nz are taken from Filgas et al. (2011). Stars from the 2MASS catalogue (Skrutskie et al. 2006) are used for the JHKs-bands.
Reference stars in the field of GRB 081007/SN 2008hw.
Reference stars in the field of GRB 101219B/SN 2010ma.
Appendix C: Black-body fits
Here we present the black-body fits for the analysed GRB-SNe, which were utilised to estimate the NIR contribution (Sect. 3.3.1).
 |
Fig. C.1
Black-body fits to the optical photometry of SN 2008hw. Colour temperatures are about 5000 K. Points with only a lower error bar are upper limits. The blue shaded region shows the area between the 1σ contours, where the central line is the best fit. |
| Open with DEXTER | |
 |
Fig. C.2
Black-body fits to the optical photometry of SN 2009nz. Colour temperatures evolve from ~7000 to ~4000 K approximately. Point, line, and region coding are the same as in Fig. C.1. |
| Open with DEXTER | |
 |
Fig. C.3
Black-body fits to the optical photometry of SN 2010ma. Colour temperatures evolve from ~6000 to ~4000 K. Point, line, and region coding are the same as in Fig. C.1. |
| Open with DEXTER | |
© ESO, 2015
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