Goal: determine parameters for the production running of ... For alpha=1, use sigma=2, time resolution = 1/128sec (small clusters and short time resolution) ...
Detected at wrong frequency (noise? ... fluctuations in the detected power ... Re-run WaveMon on-line on larger number of channels and wider frequency band. ...
After the search DSOs have identified data segments in which a ... We are considering ZM waveforms at a distance of 2 parsec (limit of sensitivity during E7) ...
We do SW injections with high statistics, to evaluate efficiency; ... which large statistics software simulations exist ... Exercise all ETGs under development ...
longish-duration, small bandwidth (chirps, ringdowns) short duration, large bandwidth (merger) ... Of course, depends on t-f resolution, which must be optimized ...
Can we see the signals in the spectrogram? Surely not, unless you really zoom in. ... Zoom in on the spectrogram. 100 Hz at 41 sec. 153 Hz at 81 sec. 235 Hz at 121 sec ...
For each triple coincidence candidate event produced by the burst pipeline ... LLO-LHO = 8, 6, 4 sec (H1-H2 together) 0.1 mHz. after r-statistic test ( 3 = 3) ...
Several lines of analysis were (internally) proposed: 15 contributions were put forward either as end-to-end analysis ... Identify main analysis directions ...
Topics in Data Analysis from Gravitational Wave Interferometers, including a ... beam from a distant spacecraft is bounced off the local proof mass before being ...
LIGO: Status, Results from the First Science Run, and Plans Albert Lazzarini LIGO Laboratory, California Institute of Technology (On behalf of the LIGO Scientific ...
Use sigmoid fitting function (Blackburn & Chatterji) ... Sigmoid fitting function turns out ok also for network efficiency curves. Solving by Monte Carlo ...
LIGO-G030546-00-D. Gravitational Wave Observations with Interferometers: Results and Prospects ... Prospects for improvement: 100-1000x from detector ...
trigger characteristics 'loudest event' upper limits. compare LIGO-Virgo to LIGO-only ... Combining Virgo WSR1 data with LIGO data gave an improved amplitude ...
... of veto channels, glitch finding method, thresholds of the veto significance' 9/24/09 ... (absGlitch) over ~3hrs of data (playground data set) 9/24/09 ...
Vetoes for E7 Inspiral Upper Limit Analysis. Overview. Goal: reduce number of inspiral candidates by vetoing times when a transient is ... A Sneak Peek at S1 ...