Project/Area Number |
18F18013
|
Research Category |
Grant-in-Aid for JSPS Fellows
|
Allocation Type | Single-year Grants |
Section | 外国 |
Research Field |
Particle/Nuclear/Cosmic ray/Astro physics
|
Research Institution | The University of Tokyo |
Principal Investigator |
カンノン キップ 東京大学, 大学院理学系研究科(理学部), 教授 (50777886)
|
Co-Investigator(Kenkyū-buntansha) |
FONG HEATHER 東京大学, 理学(系)研究科(研究院), 外国人特別研究員
|
Project Period (FY) |
2018-11-09 – 2021-03-31
|
Project Status |
Completed (Fiscal Year 2020)
|
Budget Amount *help |
¥2,100,000 (Direct Cost: ¥2,100,000)
Fiscal Year 2020: ¥400,000 (Direct Cost: ¥400,000)
Fiscal Year 2019: ¥1,100,000 (Direct Cost: ¥1,100,000)
Fiscal Year 2018: ¥600,000 (Direct Cost: ¥600,000)
|
Keywords | gravitational wave / LIGO / Virgo / black hole / neutron star / astrophysics / data analysis / detection / population model |
Outline of Annual Research Achievements |
In 2020, I worked on various projects pertaining to the analyses of the third observation run of LIGO and Virgo and first observation run of KAGRA. My contributions include creating source-dependent population models for the analyses, where the model predicts which matched-filtered waveform templates are most likely to detect the search's sources of interest (binary black holes, binary neutron stars, and neutron star black holes). The implementation of a source population model increases the sensitivity of the pipeline. In addition, I acted as a reviewer for an upcoming LIGO-Virgo-KAGRA collaboration paper that discusses the results of a search for gravitationally lensed events. I reviewed the code of the pipeline that was used to conduct the search, and I also reviewed the results that were obtained and confirmed their reproducability. I have also contributed developmental work to one of LIGO-Virgo-KAGRA's detection pipelines, GstLAL, in order to improve its efficiency and sensitivity to detecting gravitational waves.
|
Research Progress Status |
令和2年度が最終年度であるため、記入しない。
|
Strategy for Future Research Activity |
令和2年度が最終年度であるため、記入しない。
|