Random projections in gravitational-wave searches from compact binaries II: efficient reconstruction of the detection statistic
Amit Reza, Anirban Dasgupta, Anand S. Sengupta

TL;DR
This paper introduces a block-wise randomized matrix factorization method for efficient low-rank approximation of large template matrices in gravitational wave searches, significantly reducing computational costs.
Contribution
It presents a novel block-wise randomized matrix factorization algorithm and an approximate reconstruction method for detection statistics, improving efficiency in large-scale gravitational wave data analysis.
Findings
The new scheme is more efficient within the GstLAL pipeline.
Approximate reconstruction reduces total computational cost.
Combining algorithms enables more efficient online searches.
Abstract
Low-latency gravitational wave search pipelines such as GstLAL take advantage of low-rank factorization of the template matrix via singular value decomposition (SVD). With unprecedented improvements in detector bandwidth and sensitivity in advanced-LIGO and Virgo detectors, one expects several orders of magnitude increase in the size of template banks. This poses a formidable computational challenge in factorizing huge template matrices. Previously, [in Kulkarni et al. [6]], we introduced the idea of random projection (RP)-based matrix factorization as a computationally viable alternative to SVD, applicable for large template banks. This follow-up paper demonstrates the application of a block-wise randomized matrix factorization (RMF) algorithm for computing low-rank factorizations at a preset average fractional loss of SNR. This new scheme is shown to be more efficient in the context…
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Seismic Imaging and Inversion Techniques · Geophysics and Gravity Measurements
