Please do not use these results without first contacting M. Rupen. These results are preliminary, and provided here primarily to aid other observers.
All error bars are 1sigma unless otherwise noted.
Recent data (January 2005) show that the source has returned to quiescence. We are continuing regular monitoring in order to track any renewed flares, and/or brightening components distant from the core.
We reported our best VLA position for the core in ATel #304:
Please send any questions, comments, or suggestions to Michael Rupen at the e-mail address given below.
Last modified 31 January 2005
mrupen@nrao.edu