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GstLAL: A software framework for gravitational wave discovery

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arxiv 2010.05082 v1 pith:4W733E3A submitted 2020-10-10 astro-ph.IM

Kipp Cannon , Sarah Caudill , Chiwai Chan , Bryce Cousins , Jolien D. E. Creighton , Becca Ewing , Heather Fong , Patrick Godwin
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Chad Hanna Shaun Hooper Rachael Huxford Ryan Magee Duncan Meacher Cody Messick Soichiro Morisaki Debnandini Mukherjee Hiroaki Ohta Alexander Pace Stephen Privitera Iris de Ruiter Surabhi Sachdev Leo Singer Divya Singh Ron Tapia Leo Tsukada Daichi Tsuna Takuya Tsutsui Koh Ueno Aaron Viets Leslie Wade Madeline Wade
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keywords gstlalgravitational-wavedatalibraryalgorithmalthoughapproachbinary
verification ladder T0 review T1 audit T2 compute T3 formal
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The GstLAL library, derived from Gstreamer and the LIGO Algorithm Library, supports a stream-based approach to gravitational-wave data processing. Although GstLAL was primarily designed to search for gravitational-wave signatures of merging black holes and neutron stars, it has also contributed to other gravitational-wave searches, data calibration, and detector-characterization efforts. GstLAL has played an integral role in all of the LIGO-Virgo collaboration detections, and its low-latency configuration has enabled rapid electromagnetic follow-up for dozens of compact binary candidates.

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Forward citations

Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency

    gr-qc 2025-09 conditional novelty 6.0 of 10

    A new toy inspiral waveform parameterized directly by precession amplitude and frequency predicts that precession is most detectable at 'plus nulls' and in a majority of isotropic maximal-spin black-hole binaries out ...

  2. GW230814: investigation of a loud gravitational-wave signal observed with a single detector

    gr-qc 2025-09 conditional novelty 6.0 of 10

    GW230814 is a binary black hole merger seen in a single detector, yielding the first confident l=4 mode detection and a ringdown damping anomaly that noise or waveform models can explain.

  3. Searches for Binary Mergers with Sub-solar Mass Components in Data from the First Part of LIGO--Virgo--KAGRA's Fourth Observing Run

    astro-ph.HE 2026-05 conditional novelty 4.0 of 10

    No sub-solar-mass compact-binary mergers were found in LIGO O4a data, giving 90% merger-rate upper limits of 110-10000 Gpc^-3 yr^-1 and weak new dark-matter constraints.

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