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SUMMARY:Searches for GW transients with the ground-based detectors.
DTSTART;VALUE=DATE-TIME:20121016T071500Z
DTEND;VALUE=DATE-TIME:20121016T091500Z
DTSTAMP;VALUE=DATE-TIME:20200809T173144Z
UID:indico-contribution-10@cern.ch
DESCRIPTION:Speakers: KLIMENKO\, Sergey ()\nDescription: In this lecture I
give an overview of the gravitational-wave experiment \nand methods used
in the analysis of data from the ground-base detectors. \nThe purpose of
the lecture is to describe how a worldwide network of GW detectors
\nworks\, with focus on signal processing techniques and reconstruction
methods\, \nrather than to describe details of specific search algorithms
used so far in the\nGW experiment. The lecture is organized in three
parts:\n1) Short introduction into the gravitational-wave experiment.\n2)
Signal processing methods and their applications to the analysis of single
detector data\, including:\n - time-frequency transformations\n -
data conditioning with linear prediction error (LPE) filters\n -
regression of GW data\, Wiener-Kolmogorov filters\n - time-frequency
analysis\, clustering in TF domain\n - multi-resolution analysis\n3)
Analysis of data from multiple GW detectors (coherent network analysis)\,
including\n - characterization of detector networks\n - Inverse
problem for bursts\, likelihood methods\n - matched filters\, weakly
modeled and un-modeled searches \n - detection statistics\n -
reconstruction of polarization states\n - reconstruction of GW
waveforms\n - sky localization\n - factors affecting GW network
performance.\nURL: http://events.ego-
gw.it/indico/contributionDisplay.py?contribId=10&confId=1
LOCATION:EGO\, Cascina Auditorium
URL:http://events.ego-
gw.it/indico/contributionDisplay.py?contribId=10&confId=1
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