Review

1. 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 Review

2. FDS of signals from ScoX1: • 40 Hz band will be searched, projected semi-major axis, initial phase, Tobs: ~ 9 hrs, loudest event • end-to-end pipeline already tested, will 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 • needs to develop UL inference scheme • might have final results by March