Speakers
Noé Schärer
Sarah Baimukhametova
(Universite de Geneve (CH))
Description
The Einstein Telescope, the proposed next-generation European ground-based GW observatory, will dramatically increase our capability to detect GW signals. The number of detections is expected to grow from the current O(1/week) to O(1/minute), which will have a revolutionary impact on both our ability to study the dark universe and on multi-messenger science. In order to fully benefit from this potential, it is important to quickly detect GW signals, with sufficient fidelity to inform the wider multi-messenger community. Such an objective necessitates the development of new algorithms for fast signal identification; this contribution will discuss our efforts towards addressing this challenge.
Primary authors
Noé Schärer
Sarah Baimukhametova
(Universite de Geneve (CH))
Steven Schramm
(Universite de Geneve (CH))
