Physical instrumental vetoes for gravitational-wave burst triggers
P. Ajith, M. Hewitson, J. R. Smith, H. Grote, S. Hild, K. A. Strain

TL;DR
This paper introduces a physical veto strategy for gravitational-wave detectors that uses transfer functions and consistency tests to identify and exclude instrumental glitches, improving data quality with minimal false vetoes.
Contribution
The paper presents a novel, transfer function-based veto method that effectively distinguishes instrumental glitches from true gravitational-wave signals in detector data.
Findings
High veto efficiency demonstrated with hardware-injected glitches
Low accidental veto rate achieved in GEO 600 data
Method validated with hardware and GW-like injections
Abstract
We present a robust strategy to \emph{veto} certain classes of instrumental glitches that appear at the output of interferometric gravitational-wave (GW) detectors.This veto method is `physical' in the sense that, in order to veto a burst trigger, we make use of our knowledge of the coupling of different detector subsystems to the main detector output. The main idea behind this method is that the noise in an instrumental channel X can be \emph{transferred} to the detector output (channel H) using the \emph{transfer function} from X to H, provided the noise coupling is \emph{linear} and the transfer function is \emph{unique}. If a non-stationarity in channel H is causally related to one in channel X, the two have to be consistent with the transfer function. We formulate two methods for testing the consistency between the burst triggers in channel X and channel H. One method makes use of…
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