A convolutional autoencoder trained on transient gravitational wave noise (glitches) from the Gravity Spy database. Its purpose is for anomaly detection (non-anomaly=glitches, anomaly=astrophysical transient events). If successful, this will form the glitch rejection mechanism for the GW-ML burst detection pipeline MLy.
Paper on the MLy pipeline: https://arxiv.org/abs/2009.14611
Paper on the Gravity Spy database: https://iopscience.iop.org/article/10.1088/1361-6382/aa5cea
#To train the autoencoder
- Download or query the Gravity Spy database to retrieve all of the glitchs' metadata
- Feed these metadata into MLy's generator function to create timeseries of glitches with real noise
- Train the autoencoder on a given glitch type
- Test it on simulated transient events