All Tables
- Table 1:
Magnitudes of the secondary standard stars. The "-'' signs
appear where the magnitudes for the stars have not been derived either
because they were saturated in some images, which was the case of the
B and C stars, or they were faint and therefore gave large photometric
errors (>0.08). These were disregarded in the case of the U, B, and
near-IR bands of the secondary standards 1-6. The
band magnitudes
of A, B, C, and D are taken from Sahu et al. (2000).
- 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).