Swift UVOT Detection of PTF11iqb
R. M. Quimby, M. M. Kasliwal, S. Kulkarni, E. Ofek,  A. Horesh (Caltech), A. Gal-Yam, D. Xu, (Weizmann Institute)
The Swift satellite began observing PTF11iqb (ATel #3510) on July 24 and again on July 26. The UVOT data show a brightening source coincident with the location of the supernova. Including possible contamination from the host galaxy, we measure the following preliminary magnitudes:

There is no source detected by the XRT at this position. We thank the Swift team for scheduling these ToO observations.
ultra-violet,x-ray,supernovae