The MBTA pipeline for detecting compact binary coalescences in the fourth LIGO-Virgo-KAGRA observing run

Abstract In this paper, we describe the multi-band template analysis search pipeline dedicated to the detection of compact binary coalescence gravitational wave signals from the data obtained by the LIGO-Virgo-KAGRA collaboration during the fourth observing run (O4), which started in May 2023. We give details on the configuration of the pipeline and its evolution compared to the third observing run (O3). We focus here on the configuration used for the offline results of the first part of the run (O4a), which are part of the GWTC-4 catalog (in preparation). We also give a brief summary of the online configuration and highlight some of the changes implemented or considered for the second part of O4 (O4b).

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Publication Details

Journal
Classical and Quantum Gravity
Published
2025-04-29
DOI
https://doi.org/10.1088/1361-6382/add234
Citations
11
Primary Topic
Pulsars and Gravitational Waves Research
Type
article
Field-Weighted Citation Impact
12.70

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article

The MBTA pipeline for detecting compact binary coalescences in the fourth LIGO-Virgo-KAGRA observing run

G. M. Guidi, F. Aubin, L. Mobilia, A. Ouzriat et al.
11 citations
Classical and Quantum Gravity
Pulsars and Gravitational Waves Research
12.70
article

The MBTA pipeline for detecting compact binary coalescences in the fourth LIGO-Virgo-KAGRA observing run

G. M. Guidi, F. Aubin, L. Mobilia, A. Ouzriat, T. Sainrat, Frédérique Marion, I. Bentara, M. Lethuillier, V. Sordini, Vincent Juste, D. Buskulic, B. Mours, C Alléné
article en
11 citations

Abstract

Abstract In this paper, we describe the multi-band template analysis search pipeline dedicated to the detection of compact binary coalescence gravitational wave signals from the data obtained by the LIGO-Virgo-KAGRA collaboration during the fourth observing run (O4), which started in May 2023. We give details on the configuration of the pipeline and its evolution compared to the third observing run (O3). We focus here on the configuration used for the offline results of the first part of the run (O4a), which are part of the GWTC-4 catalog (in preparation). We also give a brief summary of the online configuration and highlight some of the changes implemented or considered for the second part of O4 (O4b).

Classical and Quantum GravityVol. 42(10)
Laboratoire d’Annecy de Physique des Particules (FR), Institut Pluridisciplinaire Hubert Curien (FR), Institute of Nuclear Physics of Lyon (FR), Institut de Physique des 2 Infinis de Lyon (FR)
National Science Foundation, National Research Foundation, Ministry of Education, Culture, Sports, Science and Technology, Academia Sinica, Centre National de la Recherche Scientifique, Istituto Nazionale di Fisica Nucleare, Ministry of Science and ICT, South Korea, National Science and Technology Council, Science and Technology Facilities Council, Japan Society for the Promotion of Science, Institut National de Physique Nucléaire et de Physique des Particules
Openalex Percentile: Top 1%
Pulsars and Gravitational Waves Research
12.70
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