All Tables
- Table 1:
Journal of the optical and NIR photometry of the GRB 000911
afterglow. Magnitude uncertainties are at 1
confidence level; upper
limits are at 3
confidence level. The magnitudes are not corrected
for Galactic interstellar extinction.
- Table 2:
Best-fit parameters of the GRB 000911 host galaxy obtained
with the Hyperz code. Photometric redshift errors are at 68%
confidence level. The value of the luminosity
at the knee of the
galaxies luminosity distribution (as defined by Schechter 1976; see
Sect. 4.3) is taken from Lilly et al. (1995).
- Table 3:
Best-fit parameters of the GRB 000911 afterglow light curve
in the BVRIJ bands, computed assuming a power law decay plus
a constant (host galaxy) contribution with and without the presence
of an underlying 1998bw-like SN occurring simultaneously with the GRB.
Host galaxy magnitudes reported here are not corrected for Galactic
reddening. Values within brackets are fixed in the corresponding fit.