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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

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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
Review
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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