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).