Abstract

This 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.

Highlights

  • Gravitational wave (GW) astronomy has been advancing rapidly since the first operation of the two Advanced Laser Interferometer Gravitational-wave Observatory in 2015 [1]

  • This 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 coincidence search method has long been used to search for event candidates from a detector network where high signal-to-noise ratio (SNR) triggers from individual detectors are selected first and those coincident in time are selected as candidates

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Summary

INTRODUCTION

Gravitational wave (GW) astronomy has been advancing rapidly since the first operation (referred to as O1) of the two Advanced Laser Interferometer Gravitational-wave Observatory (aLIGO) in 2015 [1]. Coherent methods have been developed for periodic GW searches [27], inspiral searches in the band of the proposed space-based interferometric detector, LISA [28,29,30], and for GRB-triggered CBC searches [31,32] It was proposed for CBC searches [33,34,35] but not widely used due to computational challenges of searching through additional parameters of source sky directions. The SVD derivation here is an extension of [40] and simplifies the expression of the coherent statistic for CBC searches It shows that output from matched filtering, i.e., the signal-to-noise ratio (SNR) time series, can be directly used and only the two parameters of sky directions need to be searched over.

PIPELINE DESCRIPTION
SPIIR method
Computational cost and GPU acceleration
Coherent network SNR
Background events from time-shift
Ranking statistic
False alarm rate estimation
Candidate veto and submission
PIPELINE PERFORMANCE AND O3 ONLINE RUN
Injection performance
O2 event search results
Latency
O3 public alerts
CONCLUSION AND DISCUSSION
Findings
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Full Text
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