Table 2: Magnitudes and corresponding fluxes of the host of GRB 990712 from all ground based observations. The fluxes in Col. 3 are obtained by correcting for a Galactic reddening of EB-V = 0.033, and offsetting to the AB system before converting the magnitudes to fluxes. The flux errors do not include the uncertainty of the Galactic reddening. The R band magnitude is consistent with that derived in Hjorth et al. (2000).
filter magnitude flux ($\mu $Jy)
U 23.12 $\pm$ 0.05 1.00 $\pm$ 0.05
B 23.36 $\pm$ 0.09 2.00 $\pm$ 0.06
V 22.39 $\pm$ 0.03 4.43 $\pm$ 0.16
R 21.84 $\pm$ 0.02 6.31 $\pm$ 0.20
I 21.41 $\pm$ 0.03 7.01 $\pm$ 0.29
J 20.81 $\pm$ 0.17 7.68 $\pm$ 1.21
H 20.25 $\pm$ 0.19 8.22 $\pm$ 1.47
Ks 19.98 $\pm$ 0.28 6.74 $\pm$ 1.71


Source LaTeX | All tables | In the text