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SPIIR online coherent pipeline to search for gravitational waves from compact binary coalescences

dc.contributor.authorChu, Qi
dc.contributor.authorKovalam, Manoj
dc.contributor.authorWen, Linqing
dc.contributor.authorSlaven-Blair, Teresa
dc.contributor.authorBosveld, Joel
dc.contributor.authorChen, Yanbei
dc.contributor.authorClearwater, P
dc.contributor.authorCodoreanu, Alex
dc.contributor.authorDu, Zhihui
dc.contributor.authorGuo, Xiangyu
dc.contributor.authorWette, Karl
dc.date.accessioned2024-03-07T23:57:56Z
dc.date.available2024-03-07T23:57:56Z
dc.date.issued2022
dc.date.updated2022-10-16T07:27:18Z
dc.description.abstractThis paper presents the Summed Parallel Infinite Impulse Response (SPIIR) pipeline used for public alerts during the third advanced LIGO and Virgo observation run (O3 run). The SPIIR pipeline uses infinite impulse response (IIR) filters to perform extremely low-latency matched filtering and this process is further accelerated with graphics processing units (GPUs). It is the first online pipeline to select candidates from multiple detectors using a coherent statistic based on the maximum network likelihood ratio statistic principle. Here we simplify the derivation of this statistic using the singular-value-decomposition (SVD) technique and show that single-detector signal-to-noise ratios from matched filtering can be directly used to construct the statistic. Coherent searches are in general more computationally challenging than coincidence searches due to extra search over sky direction parameters. The search over sky directions follows an embarrassing parallelization paradigm and has been accelerated using GPUs. The detection performance is reported using a segment of public data from LIGO-Virgo’s second observation run. We demonstrate that the median latency of the SPIIR pipeline is less than 9 seconds, and present an achievable road map to reduce the latency to less than 5 seconds. During the O3 online run, SPIIR registered triggers associated with 38 of the 56 nonretracted public alerts. The extreme low-latency nature makes it a competitive choice for joint time-domain observations, and offers the tantalizing possibility of making public alerts prior to the merger phase of binary coalescence systems involving at least one neutron star.en_AU
dc.description.sponsorshipThis work was funded by the Australian Research Council (ARC) Centre of Excellence for Gravitational Wave Discovery OzGrav under Grant No. CE170100004. K. K. is partially supported by the National Research Foundation of Korea (NRF) grant funded by the Korea government (MSIT) (Grant No. NRF-2020R1C1C1005863). T. G. F. L. was partially supported by grants from the Research Grants Council of the Hong Kong (Project No. CUHK14306419 and No. CUHK14306218), Research Committee of the Chinese University of Hong Kong and the Croucher Foundation of Hong Kong. A. Sengupta thanks the Department of Science and Technology for their ICPS cluster Grant No. DST/ICPS/Cluster/ Data_Science/2018/General/T-150. We wish to acknowledge Tom Almeida, Andrew Munt, Zhaohong Peng, Han-Shiang Kuo, Fengli Lin, Guo Chin Liu for helpful discussions on the improvement of the work. This work used the computer resources of the LIGO CIT (Caltech) computer cluster and OzStar computer cluster at Swinburne University of Technology. LIGO CIT cluster is funded by National Science Foundation Grants No. PHY-0757058 and No. PHY-0823459. The OzSTAR program receives funding in part from the Astronomy National Collaborative Research Infrastructure Strategy (NCRIS) allocation provided by the Australian Government. We wish to thank Stuart Anderson, Jarrod Hurley for the great help to use the clusters. This research used data obtained from the Gravitational Wave Open Science Center [58], a service of LIGO Laboratory, the LIGO Scientific Collaboration and the Virgo Collaboration. LIGO is funded by the U.S. National Science Foundation. Virgo is funded by the French Centre National de Recherche Scientifique (CNRS), the Italian Istituto Nazionale della Fisica Nucleare (INFN) and the Dutch Nikhef, with contributions by Polish and Hungarian institutes. This research used the injection sets generated by the rates and population group of the LIGO Scientific Collaboration. We acknowledge the GstLAL Team for the GstLAL library for several modules used in this work.en_AU
dc.format.mimetypeapplication/pdfen_AU
dc.identifier.issn2470-0010en_AU
dc.identifier.urihttp://hdl.handle.net/1885/315818
dc.language.isoen_AUen_AU
dc.provenancehttps://v2.sherpa.ac.uk/id/publication/32264..."The Published Version can be archived in an Institutional Repository" from SHERPA/RoMEO site (as at 8/03/2024).en_AU
dc.publisherAmerican Physical Societyen_AU
dc.relationhttp://purl.org/au-research/grants/arc/CE170100004en_AU
dc.rights© 2022 American Physical Societyen_AU
dc.sourcePhysical Review Den_AU
dc.titleSPIIR online coherent pipeline to search for gravitational waves from compact binary coalescencesen_AU
dc.typeJournal articleen_AU
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.issue2en_AU
local.bibliographicCitation.lastpage024023-17en_AU
local.bibliographicCitation.startpage024023-1en_AU
local.contributor.affiliationChu, Qi, The University of Western Australiaen_AU
local.contributor.affiliationKovalam, Manoj, The University of Western Australiaen_AU
local.contributor.affiliationWen, Linqing, The University of Western Australiaen_AU
local.contributor.affiliationSlaven-Blair, Teresa, The University of Western Australiaen_AU
local.contributor.affiliationBosveld, Joel, University of Western Australiaen_AU
local.contributor.affiliationChen, Yanbei, California Institute of Technologyen_AU
local.contributor.affiliationClearwater, P, University of Melbourneen_AU
local.contributor.affiliationCodoreanu, Alex, The University of Western Australiaen_AU
local.contributor.affiliationDu, Zhihui, New Jersey Institute of Technologyen_AU
local.contributor.affiliationGuo, Xiangyu, Tsinghua Universityen_AU
local.contributor.affiliationWette, Karl, College of Science, ANUen_AU
local.contributor.authoruidWette, Karl, u4090078en_AU
local.description.notesImported from ARIESen_AU
local.identifier.absfor510100 - Astronomical sciencesen_AU
local.identifier.absseo280120 - Expanding knowledge in the physical sciencesen_AU
local.identifier.ariespublicationa383154xPUB24698en_AU
local.identifier.citationvolume105en_AU
local.identifier.doi10.1103/PhysRevD.105.024023en_AU
local.identifier.scopusID2-s2.0-85122736589
local.publisher.urlhttps://journals.aps.org/en_AU
local.type.statusPublished Versionen_AU

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