2 citations · 3 across the 6 of their papers we have counts for
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Scattered light noise at LIGO Livingston Observatory during O4
Debasmita Nandi, Anamaria Effler, Siddharth Soni +6
Scattered light is one of the most common sources of noise in the LIGO gravitational wave detectors. Light scattering is a highly non-linear process through which motion at low fre…
The Sound of Noise: Leveraging the Inductive Bias of Pre-trained Audio Transformers for Glitch Identification in LIGO
Suyash Deshmukh, Chayan Chatterjee, Abigail Petulante +2
Transient noise artifacts, or glitches, fundamentally limit the sensitivity of gravitational-wave (GW) interferometers and can mimic true astrophysical signals, particularly the sh…
An Analysis of LIGO Glitches Using t-SNE During the First Part of the Fourth LIGO-Virgo-KAGRA Observing Run
Tabata Aira Ferreira, Gabriela González, Osvaldo Salas
This paper presents an analysis of noise transients observed in LIGO data during the first part of the fourth observing run, using the unsupervised machine learning technique t-dis…
Using t-SNE for characterizing glitches in LIGO detectors
Tabata Aira Ferreira, Gabriela González
Glitches are non-Gaussian noise transients originating from environmental and instrumental sources that contaminate data from gravitational wave detectors. Some glitches can even m…