Review production of 30min calibrated SFTs well under way (see talks by V.Dergachev., X. Siemens in ASIS/DetChar). Also expect calibrated h(t) in the next 2 weeks. TDS of signals from known pulsars: changes wrt S1 analysis in: noise estimation phase evolution model for Crab now reliable ULs for ~30 known pulsars now preliminary ULs (correct within sqrt(2) for remaining 9 All-sky, wide-frequency FDS, Tobs ~ ½ day: changes wrt S1: robust wide band noise estimation event identification procedure event shape test all machinery is in place, need to run end-to-end pipeline on final data set and entire parameter space GC, wide-frequency FDS, Tobs: entire run will exploit ~ 1000 CPUs for 1 month (AEI, Birmingham, Caltech, Cardiff, ISI, UWM) will begin next week at SC03 conference

FDS of signals from ScoX1: 80 Hz band will be searched, projected semi-major axis, initial phase, Tobs: ~ ½ day, loudest event end-to-end pipeline already tested, might include a c2 test on candidates expect results by the end of the year Hough transform: all-sky, 1 spin-down parameter search, Tobs: entire S2 run, loudest event pipeline in place, including monte carlo injections for determining UL detection statistic all machinery is in place, need to run end-to-end pipeline on final data set and entire parameter space Stack-slide search: debugging sliding needs to develop UL inference scheme might have final results by March Unbiased search: developed power statistic from 30 min SFTs