Conveners
Session II
- Antoni Ramos Buades (University of the Balearic Islands)
The Einstein Telescope (ET), a third-generation gravitational-wave (GW) observatory, will extend the sensitivity and bandwidth of current detectors, enabling observations from ~1 Hz and vastly increasing the detection rate of compact binary coalescences (CBCs). This leap in capability introduces new data analysis challenges, including increased rates of overlapping signals that can generate...
The sensitivity of Gravitational Waves (GW) interferometers is limited by noise. Non-Gaussian transient noise artifacts, also known as glitches, are particularly challenging due to their similarity with astrophysical signals in the time and frequency domains; for this reason noise reduction and subtraction is one of the most important and challenging activities in GW research. Within the...
Gravitational wave data are often contaminated by transient noise artifacts, called "glitches", which can mimic astrophysical signals and interfere with their detection. When represented in the time-frequency domain, glitches show peculiar morphologies, which allow their categorization into distinct families. As it is expected that glitches which share a similar morphology also share the same...
