Pith. sign in

REVIEW 2 cited by

DQSEGDB: A time-interval database for storing gravitational wave observatory metadata

Not yet reviewed by Pith; the record is open.

Re-run · record.json Download PDF Read on arXiv ↗

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 2008.11316 v1 pith:WQ2VFQDM submitted 2020-08-26 astro-ph.IM

Ryan P. Fisher , Gary Hemming , Marie-Anne Bizouard , Duncan A. Brown , Peter F. Couvares , Florent Robinet , Didier Verkindt This is my paper · ORCID
classification astro-ph.IM
keywords dqsegdbdatabasegravitationalmetadatadetectorobservatoryroughlystoring
verification ladder T0 review T1 audit T2 compute T3 formal

Signed reviews

No signed human review yet.

0 comments
read the original abstract

The Data Quality Segment Database (DQSEGDB) software is a database service, backend API, frontend graphical web interface, and client package used by the Laser Interferometer Gravitational-Wave Observatory (LIGO), Virgo, GEO600 and the Kamioka Gravitational wave detector for storing and accessing metadata describing the status of their detectors. The DQSEGDB has been used in the analysis of all published detections of gravitational waves in the advanced detector era. The DQSEGDB currently stores roughly 600 million metadata entries and responds to roughly 600,000 queries per day with an average response time of 0.223 ms.

Discussion (0). Continue with ORCID to comment.

Forward citations

Cited by 2 Pith papers

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

  1. GWTC-4.0: Updating the Gravitational-Wave Transient Catalog with Observations from the First Part of the Fourth LIGO-Virgo-KAGRA Observing Run

    gr-qc 2025-08 accept novelty 6.0 of 10

    The LIGO-Virgo-KAGRA collaboration adds 128 new compact binary merger candidates from O4a, including the heaviest binary black hole yet observed (total mass about 236 solar masses) and the first black hole mergers wit...

  2. 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.

Pith tools