However, it is available through the USNO PMM pixel database. No candidate was found above the POSS-II plate limit. The two deep exposure sets from USNO were blinked to look for transients below the POSS-II plate limit. Refinement of this photometry will be performed in late April if an OT is discovered. Further data analysis is in progress.
Further refinements are still possible.
The data analysis is in progress and an image will be put on the laboratory web page when available. We also intend to continue observations of the optical counterpart tonight as well. This message may be cited. No astronomical filter was used during these observations. Further analysis is in progress.