Good day!
    My initial work was on identifying outlier frequencies in S5 and S6. PowerFlux is finishing up on the S6 run with more reslts to be analyzed. After a summer at Virgo using their noise monitoring tool NoEMi, I have been comparing its utility and effectiveness at identifying noise lines compared to some of LIGO's tools, namely STAMP, Fscan, and coherence. I also examine optimal telescopes to use for searching for X-ray afterglows of short gamma-ray bursts in anticipition for LIGO's detection of gravitational waves from NS-NS and NS-BH sources.