Download presentation
Presentation is loading. Please wait.
Published byAlyson Porter Modified over 9 years ago
1
Soma Mukherjee, GWDAW7, Kyoto, Japan, 19/12/02, LIGO-G030166-00-Z1 Robust Detection of Noise Floor Drifts in Interferometric Data Soma Mukherjee Max Planck Institut fuer Gravitationsphysik Golm, Germany. GWDAW7, Kyoto, Japan, 19/12/02
2
Soma Mukherjee, GWDAW7, Kyoto, Japan, 19/12/02, LIGO-G030166-00-Z2 Motivation : Interferometric data has three components : Lines, transients, noise floor. Study of a change in any one of these without elimination of the other two will cause interference. Lines dominate. Presence of transients change the central tendency. “SLOW” nonstationarity of noise floor interesting in the analysis of several astrophysical searches, e.g. Externally triggered search.
3
Soma Mukherjee, GWDAW7, Kyoto, Japan, 19/12/02, LIGO-G030166-00-Z3 Methods : Running Median. Computation of : G(m)=V(Z t+m – Z t )/V(Z t+1 – Z t ) Z t : t th sample of a timeseries. m: Lag.
4
Soma Mukherjee, GWDAW7, Kyoto, Japan, 19/12/02, LIGO-G030166-00-Z4 Sequence : Low pass and resample Estimate spectral noise floor using Running Median Design FIR Whitening filter. Whiten data. Clean lines. Highpass. Compute Running Median of the squared timeseries. Construct Variograms. Thresholds set by Simulation.
5
Soma Mukherjee, GWDAW7, Kyoto, Japan, 19/12/02, LIGO-G030166-00-Z5
6
6
7
7
8
8
9
9
10
10
11
Soma Mukherjee, GWDAW7, Kyoto, Japan, 19/12/02, LIGO-G030166-00-Z11
12
Soma Mukherjee, GWDAW7, Kyoto, Japan, 19/12/02, LIGO-G030166-00-Z12
13
Soma Mukherjee, GWDAW7, Kyoto, Japan, 19/12/02, LIGO-G030166-00-Z13
14
Soma Mukherjee, GWDAW7, Kyoto, Japan, 19/12/02, LIGO-G030166-00-Z14
15
Soma Mukherjee, GWDAW7, Kyoto, Japan, 19/12/02, LIGO-G030166-00-Z15
16
Soma Mukherjee, GWDAW7, Kyoto, Japan, 19/12/02, LIGO-G030166-00-Z16
17
Soma Mukherjee, GWDAW7, Kyoto, Japan, 19/12/02, LIGO-G030166-00-Z17
18
Soma Mukherjee, GWDAW7, Kyoto, Japan, 19/12/02, LIGO-G030166-00-Z18
19
Soma Mukherjee, GWDAW7, Kyoto, Japan, 19/12/02, LIGO-G030166-00-Z19 Future : `To be run on full S1 data (LIGO/GEO). More quantification of the Running Median and variogram. To be tested on bandlimited data. Automation and incorporation in the DCR underway.
Similar presentations
© 2024 SlidePlayer.com Inc.
All rights reserved.