We have continued our near-infrared observations of the "L" impact site at Whately observatory with an intent of producing a continuous light curve at 2.23 - 2.29um. We have also taken occasional observations at 1.64, 2.12, 2.16, and 2.29um.

In addition, we just looked through the 4" refactor which serves as the finder for our 16" telescope. The "L" impact site, which is now at the center of the disk, appears as a distinct dark spot. We also believe we can see site "G" as a slightly more diffuse spot to the east.

Images from the NICMASS observations will be available shortly at

http://scruffy.phast.umass.edu/Whately/sl9.html