  At the time of this conference, in June 2002, The LIGO Science Collaboration
was getting ready to perform its first Science Run, where data will be taken
with all three LIGO detectors. We describe here the status of the LIGO
detectors as of February 2003, their performance during the ``Engineering Run''
E7 (Dec 28'01-Jan 14'02) and subsequent Science Runs in 2002/3. We also
describe ongoing efforts on data analysis for setting upper limits of different
gravitational wave sources.
