Abstract (may include machine translation)
The understanding of noise in interferometric gravitational wave detectors is fundamental in terms of both enabling prompt reactions in the mitigation of noise disturbances and in the establishment of appropriate data-cleaning strategies. Monitoring tools to perform online and offline noise analysis in areas such as transient signal detection, line identification algorithms and coherence are used to characterise the Virgo detector noise. In this paper, we describe the framework into which these tools are integrated - the Noise Monitor Application Programming Interface (NMAPI) - and provide examples of its application.
| Original language | English |
|---|---|
| Article number | 012024 |
| Journal | Journal of Physics: Conference Series |
| Volume | 363 |
| Issue number | 1 |
| DOIs | |
| State | Published - 2012 |
| Externally published | Yes |
| Event | 9th Edoardo Amaldi Conference on Gravitational Waves, Amaldi 9 and the 2011 Numerical Relativity - Data Analysis Meeting, NRDA 2011 - Cardiff, United Kingdom Duration: 10 Jul 2011 → 15 Jul 2011 |
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