Year-end Sale % OFF 
Abstract
Existing observations of the universe mostly come from electromagnetic (EM) waves, representing so-called multi-wavelength astronomy. In order to enable multi-messenger astronomy, direct detection of gravitational waves (GWs) has to be processed in nearly real time. In this work, we discuss algorithm and infrastructure challenges for GW burst (GWB) search to enable multi-messenger astronomy involving GWs. A real-time computing infrastructure for LIGO (Laser Interferometer Gravitational-wave Observatory) GWB data analysis is presented, using advanced computing technologies.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
