This data set contains all classifications that the Gravity Spy Machine Learning model for LIGO glitches from the first three observing runs (O1, O2 and O3, where O3 is split into O3a and O3b). Gravity Spy classified all noise events identified by the Omicron trigger pipeline in which Omicron identified that the signal-to-noise ratio was above 7.5 and the peak frequency of the noise event was between 10 Hz and 2048 Hz. To classify noise events, Gravity Spy made Omega scans of every glitch consisting of 4 different durations, which helps capture the morphology of noise events that are both short and long in duration. There are 22 classes used for O1 and O2 data (including No_Glitch and None_of_the_Above), while there are two additional clas...
Data streams of gravitational-wave detectors are polluted by transient noise features, or "glitches"...
With the first direct detection of gravitational waves, the Advanced Laser Interferometer Gravitati...
The noise of gravitational-wave (GW) interferometers limits their sensitivity and impacts the data q...
Understanding the noise in gravitational-wave detectors is central to detecting and interpreting gra...
This dataset contains machine learning and volunteer classifications from the Gravity Spy project. I...
(abridged for arXiv) With the first direct detection of gravitational waves, the Advanced Laser Inte...
With the first direct detection of gravitational waves, the advanced laser interferometer gravitatio...
We present the first version of the training set used in the Gravity Spy citizen science project. Th...
The observation of gravitational waves is hindered by the presence of transient noise (glitches). We...
We investigate the use of Convolutional Neural Networks (including the modern ConvNeXt network famil...
The observation of gravitational waves is hindered by the presence of transient noise (glitches). We...
The sensitivity of searches for astrophysical transients in data from the Laser Interferometer Gravi...
We investigate the use of convolutional neural networks (including the modern ConvNeXt network famil...
The observation of gravitational waves from compact binary coalescences by LIGO and Virgo has begun ...
The observation of gravitational waves from compact binary coalescences by LIGO and Virgo has begun ...
Data streams of gravitational-wave detectors are polluted by transient noise features, or "glitches"...
With the first direct detection of gravitational waves, the Advanced Laser Interferometer Gravitati...
The noise of gravitational-wave (GW) interferometers limits their sensitivity and impacts the data q...
Understanding the noise in gravitational-wave detectors is central to detecting and interpreting gra...
This dataset contains machine learning and volunteer classifications from the Gravity Spy project. I...
(abridged for arXiv) With the first direct detection of gravitational waves, the Advanced Laser Inte...
With the first direct detection of gravitational waves, the advanced laser interferometer gravitatio...
We present the first version of the training set used in the Gravity Spy citizen science project. Th...
The observation of gravitational waves is hindered by the presence of transient noise (glitches). We...
We investigate the use of Convolutional Neural Networks (including the modern ConvNeXt network famil...
The observation of gravitational waves is hindered by the presence of transient noise (glitches). We...
The sensitivity of searches for astrophysical transients in data from the Laser Interferometer Gravi...
We investigate the use of convolutional neural networks (including the modern ConvNeXt network famil...
The observation of gravitational waves from compact binary coalescences by LIGO and Virgo has begun ...
The observation of gravitational waves from compact binary coalescences by LIGO and Virgo has begun ...
Data streams of gravitational-wave detectors are polluted by transient noise features, or "glitches"...
With the first direct detection of gravitational waves, the Advanced Laser Interferometer Gravitati...
The noise of gravitational-wave (GW) interferometers limits their sensitivity and impacts the data q...