Curriculum Vitaes
Profile Information
- Affiliation
- Institute of Space and Astronautical Science, Japan Aerospace Exploration AgencyGraduate School of Science Department of Astronomy, The University of Tokyo
- J-GLOBAL ID
- 200901049964309113
- researchmap Member ID
- 5000001980
- External link
Research Interests
5Research Areas
2Research History
1-
Oct, 2017 - Present
Major Papers
152-
Applied Optics, Aug 8, 2024
-
Journal of Astronomical Telescopes, Instruments, and Systems, 9(02), Apr 19, 2023
-
Journal of Astronomical Telescopes, Instruments, and Systems, 9(02), Apr 12, 2023
-
Progress of Theoretical and Experimental Physics, 2023(4), Nov 21, 2022Abstract LiteBIRD, the Lite (Light) satellite for the study of B-mode polarization and Inflation from cosmic background Radiation Detection, is a space mission for primordial cosmology and fundamental physics. The Japan Aerospace Exploration Agency (JAXA) selected LiteBIRD in May 2019 as a strategic large-class (L-class) mission, with an expected launch in the late 2020s using JAXA’s H3 rocket. LiteBIRD is planned to orbit the Sun–Earth Lagrangian point L2, where it will map the cosmic microwave background polarization over the entire sky for three years, with three telescopes in 15 frequency bands between 34 and 448 GHz, to achieve an unprecedented total sensitivity of $2.2\, \mu$K-arcmin, with a typical angular resolution of 0.5○ at 100 GHz. The primary scientific objective of LiteBIRD is to search for the signal from cosmic inflation, either making a discovery or ruling out well-motivated inflationary models. The measurements of LiteBIRD will also provide us with insight into the quantum nature of gravity and other new physics beyond the standard models of particle physics and cosmology. We provide an overview of the LiteBIRD project, including scientific objectives, mission and system requirements, operation concept, spacecraft and payload module design, expected scientific outcomes, potential design extensions, and synergies with other projects.
-
Space Telescopes and Instrumentation 2022: Optical, Infrared, and Millimeter Wave, Aug 27, 2022
-
Space Telescopes and Instrumentation 2022: Optical, Infrared, and Millimeter Wave, Aug 27, 2022
-
SPACE TELESCOPES AND INSTRUMENTATION 2022: OPTICAL, INFRARED, AND MILLIMETER WAVE, 12180, 2022
-
Proceedings of SPIE - The International Society for Optical Engineering, 11453, 2020
-
Proceedings of SPIE - The International Society for Optical Engineering, 11453, 2020
-
IEEE Transactions on Terahertz Science and Technology, 9(6) 598-605, Nov, 2019 Peer-reviewed
-
Journal of Astronomical Telescopes, Instruments, and Systems, 5(4), Oct 1, 2019 Peer-reviewed
-
Proceedings of SPIE - The International Society for Optical Engineering, 10698, 2018 Peer-reviewed
-
IEEE Transactions on Applied Superconductivity, 25(3), Jun 1, 2015 Peer-reviewed
Misc.
215-
IEEE Transactions on Nuclear Science, 40(4) 890-898, Aug, 1993 Peer-reviewed
-
IEEE Transactions on Nuclear Science, 40(2) 204-207, Apr, 1993 Peer-reviewed
-
Meeting Abstracts of the Physical Society of Japan, 48 138-138, 1993
-
COMPTON GAMMA-RAY OBSERVATORY, 280 355-359, 1993 Peer-reviewed
-
AIP Conference Proceedings, 280 213-217, 1993 Peer-reviewed
-
AIP Conference Proceedings, 280 523-527, 1993 Peer-reviewed
-
IEEE Transactions on Nuclear Science, 39(5) 1316-1320, Oct, 1992 Peer-reviewed
-
Astrophysical Journal, 397(2 PART 2) L83-L86, Oct 1, 1992 Peer-reviewed
-
30 61-81, Feb, 1992We have developed a new kind of phoswih counters (the well-type phoswich counter) that is capable of detecting very low flux hard X-rays/gamma-rays (60-800 keV) from astronomical object. We flew the first prototype detector system (Welcome-1) from Cachoeira Paulista, Brazil in November 1990. The objective was to detect ^<57>Co (122,136keV) and continuum emission from SN1987A. The background spectrum taken at an altitude of 4g/cm^2 indicates that the 3σ sensitivity reaches ∿a few×10^<-6>/cm^2/s/keV and ∿10^<-4>/cm^2/s by 10^4s observation for the continuum spectrum and line spectrum respectively.
-
Meeting Abstracts of the Physical Society of Japan, 47 72-72, 1992
-
Proceedings of SPIE - The International Society for Optical Engineering, 1734 44-55, 1992 Peer-reviewed
-
Proceedings of SPIE - The International Society for Optical Engineering, 1734 2-13, 1992 Peer-reviewed
-
Meeting Abstracts of the Physical Society of Japan, 1991 83-83, 1991
-
Meeting Abstracts of the Physical Society of Japan, 45 68-68, 1990
Presentations
78Teaching Experience
2-
Oct, 2022 - Jan, 2023High energy astrophysics (The University of Tokyo)
-
Jul, 2020 - Aug, 2020Space astronomy (sokendai)
Research Projects
9-
Grants-in-Aid for Scientific Research, Japan Society for the Promotion of Science, Jun, 2023 - Mar, 2027
-
Grants-in-Aid for Scientific Research, Japan Society for the Promotion of Science, Apr, 2023 - Mar, 2027
-
Grants-in-Aid for Scientific Research, Japan Society for the Promotion of Science, Apr, 2023 - Mar, 2027
-
Grants-in-Aid for Scientific Research Grant-in-Aid for Scientific Research (A), Japan Society for the Promotion of Science, Apr, 2017 - Mar, 2021
-
Grants-in-Aid for Scientific Research Grant-in-Aid for Scientific Research on Innovative Areas (Research in a proposed research area), Japan Society for the Promotion of Science, Jun, 2015 - Mar, 2020
Industrial Property Rights
3Social Activities
1● 指導学生等の数
1-
Fiscal Year2021年度(FY2021)Doctoral program1Master’s program1Internship students9
● 指導学生の表彰・受賞
1-
Student NameHayato TAKAKURAStudent affiliation東京大学AwardB-mode from spaceDate2019-12-5
● 専任大学名
1-
Affiliation (university)東京大学（University of Tokyo)
