Project/Area Number |
23K20871
|
Research Category |
Grant-in-Aid for Scientific Research (B)
|
Allocation Type | Multi-year Fund |
Section | 一般 |
Review Section |
Basic Section 16010:Astronomy-related
|
Research Institution | National Astronomical Observatory of Japan |
Principal Investigator |
SHAN Wenlei 国立天文台, 先端技術センター, 准教授 (60792570)
|
Co-Investigator(Kenkyū-buntansha) |
江崎 翔平 国立天文台, 先端技術センター, 研究技師 (40794508)
田村 友範 国立天文台, 先端技術センター, 技師 (90897828)
|
Project Period (FY) |
2024-04-01 – 2026-03-31
|
Project Status |
Granted (Fiscal Year 2024)
|
Budget Amount *help |
¥6,500,000 (Direct Cost: ¥5,000,000、Indirect Cost: ¥1,500,000)
Fiscal Year 2025: ¥3,770,000 (Direct Cost: ¥2,900,000、Indirect Cost: ¥870,000)
Fiscal Year 2024: ¥2,730,000 (Direct Cost: ¥2,100,000、Indirect Cost: ¥630,000)
|
Keywords | Focal plane array / SIS mixer / Radio astronomy / planar OMT |
Outline of Research at the Start |
This research is relevant to a new technological approach to constructing sub-mm heterodyne focal plane arrays for radioastronomical observation. This approach is characterized by the adoption of superconducting monolithic microwave integrated circuits (MMICs) and hybrid planar integration (HPI) schemes.
|