I've placed on http://ftp.nofs.navy.mil/pub/outgoing/aah/grb/991216.txt a diary of the observations for this bright gamma-ray burst. Note that the burst was reasonably well localized by 6 hours after the burst, but no optical observatory has reported an image of the optical transient earlier than 11 hours after the burst. By this time, the GRB had faded to R=18.8. Note also that almost any amateur with a telescope with an unfiltered CCD could have observed this optical transient. I posted information early enough for most Europeans to have tried, and the source was still 'bright' by the time it was viewable in the U.S. Did anyone detect the transient? The HETE-II satellite is due to be launched in about a month. This satellite will deliver arcmin positions within seconds after a burst. The regime from burst until about 8hrs after the burst is largely unexplored, and amateurs with quick response may be able to contribute important observations, especially if they can use a standard filter like R. The AAVSO is already discussing involvement with Marshall Space Flight Center. This is not the usual type of variable star observations that maillist participants are used to, yet this is not that different than novae or supernovae observations. I hope some readers get involved! There are only about a dozen professional observatories that can contribute data on a given burst, and often they get clouded out or have the wrong instrumentation on the telescope. Arne