Pith. sign in

REVIEW 1 cited by

Noise in the LIGO Livingston Gravitational Wave Observatory due to Trains

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 2304.07477 v1 pith:NRXHHB3Y submitted 2023-04-15 astro-ph.IM

Jane Glanzer , Siddharth Soni , Jaidyn Spoon , Anamaria Effler , Gabriela González This is my paper · ORCID
classification astro-ph.IM
keywords ligogravitationallivingstonnoiseseismictrainswaveband
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

Environmental seismic disturbances limit the sensitivity of LIGO gravitational wave detectors. Trains near the LIGO Livingston detector produce low frequency (0.5-10 Hz) ground noise that couples into the gravitational wave sensitive frequency band (10-100 Hz) through light reflected in mirrors and other surfaces. We investigate the effect of trains during the Advanced LIGO third observing run, and propose a method to search for narrow band seismic frequencies responsible for contributing to increases in scattered light. Through the use of the linear regression tool Lasso (least absolute shrinkage and selection operator) and glitch correlations, we identify the most common seismic frequencies that correlate with increases in detector noise as 0.6-0.8 Hz, 1.7-1.9 Hz, 1.8-2.0 Hz, and 2.3-2.5 Hz in the LIGO Livingston corner station.

Discussion (0). Continue with ORCID to comment.

Forward citations

Cited by 1 Pith paper

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

  1. Adaptive cancellation of mains power interference in continuous gravitational wave searches with a hidden Markov model

    gr-qc 2024-12 conditional novelty 5.0 of 10

    An adaptive recursive least squares filter, referenced to mains-power monitor channels, suppresses the 60 Hz line in LIGO data so that a hidden Markov model can recover an injected, frequency-wandering continuous wave signal.

Pith tools