Difference between revisions of "Members"
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File:JanHarms.jpg|'''Jan Harms'''. Full professor working on instrument science of current and future GW detectors, and data analysis of modeled and unmodeled GW signals. | File:JanHarms.jpg|'''Jan Harms'''. Full professor working on instrument science of current and future GW detectors, and data analysis of modeled and unmodeled GW signals. | ||
File:Marica.jpg|'''Marica Branchesi'''. Full professor working on multi-messenger astrophysics and observations with gravitational-waves. | File:Marica.jpg|'''Marica Branchesi'''. Full professor working on multi-messenger astrophysics and observations with gravitational-waves. | ||
| − | File:AndreaMaselli.jpg|'''Andrea Maselli'''. | + | File:AndreaMaselli.jpg|'''Andrea Maselli'''. Associate professor working on LISA and ET signal modeling and testing GR. |
File:Gor.jpg|'''Gor Oganesyan'''. Assistant professor working on the theoretical modeling and analysis of GRB signals and afterglows. | File:Gor.jpg|'''Gor Oganesyan'''. Assistant professor working on the theoretical modeling and analysis of GRB signals and afterglows. | ||
File:Manuel_2023.jpg|'''Manuel Arca Sedda'''. Assistant professor whose main research focuses on the formation and evolution of compact binary objects and intermediate-mass black holes and their role in GW astronomy, leveraging on a combination of theoretical/semi-analytical approaches, numerical simulations exploiting high-performance computing, and data analysis. | File:Manuel_2023.jpg|'''Manuel Arca Sedda'''. Assistant professor whose main research focuses on the formation and evolution of compact binary objects and intermediate-mass black holes and their role in GW astronomy, leveraging on a combination of theoretical/semi-analytical approaches, numerical simulations exploiting high-performance computing, and data analysis. | ||
Revision as of 14:08, 27 March 2025
Current gravitational-wave group at Gran Sasso Science Institute
- JanHarms.jpg
Jan Harms. Full professor working on instrument science of current and future GW detectors, and data analysis of modeled and unmodeled GW signals.
Manuel Arca Sedda. Assistant professor whose main research focuses on the formation and evolution of compact binary objects and intermediate-mass black holes and their role in GW astronomy, leveraging on a combination of theoretical/semi-analytical approaches, numerical simulations exploiting high-performance computing, and data analysis.