Jump to content
Main menu
Main menu
move to sidebar
hide
Navigation
Pop Culture
Art & Architecture
Comics
Comic Issues
Disney
Japanifornia Locations
Fictional Characters
Gaijin in Japan
Literature
Movies
Music
Television
Video Games
Real Life
Culture
Glossary
Hāfu
Nihonjin
Nikkei
Nikkei who were interned
Tropes
Wiki Decades
The 1940s
The 1950s
The 1960s
The 1970s
The 1980s
The 1990s
The 2000s
The 2010s
The 2020s
Special
List Files
All Categories
Needs Love
Wanted Pages
Edit Toolbar
Check It Out
Random page
Recent changes
Help about MediaWiki
J-Wiki
Search
Search
Log in
Personal tools
Log in
Pages for logged out editors
learn more
Contributions
Talk
Editing
Samaya Nissanke
Page
Discussion
English
Read
Edit
View history
Tools
Tools
move to sidebar
hide
Actions
Read
Edit
View history
General
What links here
Related changes
Special pages
Page information
Warning:
You are not logged in. Your IP address will be publicly visible if you make any edits. If you
log in
or
create an account
, your edits will be attributed to your username, along with other benefits.
Anti-spam check. Do
not
fill this in!
Samaya Michiko Nissanke is an astrophysicist and the spokesperson for the GRAPPA Centre for Excellence in Gravitation and Astroparticle Physics at the University of Amsterdam. She works on gravitational-wave astrophysics and has played a founding role in the emerging field of multi-messenger astronomy. She was a pivotal figure in the discovery paper of the first binary neutron star merger, GW170817, seen in gravitational waves and electromagnetic radiation. Nissanke was born in London to a Sri-Lankan father and a Japanese mother. She completed her Bachelor's and Master's degree in Physics at the University of Cambridge. She joined the Paris Observatory for her postgraduate studies. Nissanke earned her PhD in analytical relativity at the Institut d'astrophysique de Paris in 2007 with a thesis titled Aspects théoriques de la forme des ondes gravitationnelles pour les phases spiralante et de fusion des systèmes binaires compacts (Theoretical aspects of the shape of gravitational waves for the spiraling and merging phases of compact binary systems). [[Category:Hāfu]] [[Category:STEM]] [[Category:🇯🇵🇱🇰]]
Summary:
Please note that all contributions to J-Wiki may be edited, altered, or removed by other contributors. If you do not want your writing to be edited mercilessly, then do not submit it here.
You are also promising us that you wrote this yourself, or copied it from a public domain or similar free resource (see
J-Wiki:Copyrights
for details).
Do not submit copyrighted work without permission!
Cancel
Editing help
(opens in new window)
Toggle limited content width