NICE: A Web-Based Tool for the Characterization of Transient Noise in Gravitational Wave Detectors

Author:

Sorrentino Nunziato12ORCID,Razzano Massimiliano12ORCID,Di Renzo Francesco3ORCID,Fidecaro Francesco12ORCID,Hemming Gary4ORCID

Affiliation:

1. Department of Physics, Università di Pisa, I-56127 Pisa, Italy

2. Sezione di Pisa, INFN, I-56127 Pisa, Italy

3. Université Lyon, Université Claude Bernard Lyon 1, CNRS, IP2I Lyon/IN2P3, UMR 5822, F-69622 Villeurbanne, France

4. European Gravitational Observatory (EGO), Cascina, I-56021 Pisa, Italy

Abstract

NICE—Noise Interactive Catalogue Explorer—is a web service developed for rapid-qualitative glitch analysis in gravitational wave data. Glitches are transient noise events that can smother the gravitational wave signal in data recorded by gravitational wave interferometer detectors. NICE provides interactive graphical tools to support detector noise characterization activities, in particular, the analysis of glitches from past and current observing runs, passing from glitch population visualization to individual glitch characterization. The NICE back-end API consists of a multi-database structure that brings order to glitch metadata generated by external detector characterization tools so that such information can be easily requested by gravitational wave scientists. Another novelty introduced by NICE is the interactive front-end infrastructure focused on glitch instrumental and environmental origin investigation, which uses labels determined by their time–frequency morphology. The NICE domain is intended for integration with the Advanced Virgo, Advanced LIGO, and KAGRA characterization pipelines and it will interface with systematic classification activities related to the transient noise sources present in the Virgo detector.

Funder

European Union

Publisher

MDPI AG

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