Budget Amount *help |
¥25,350,000 (Direct Cost: ¥19,500,000、Indirect Cost: ¥5,850,000)
Fiscal Year 2009: ¥1,170,000 (Direct Cost: ¥900,000、Indirect Cost: ¥270,000)
Fiscal Year 2008: ¥11,830,000 (Direct Cost: ¥9,100,000、Indirect Cost: ¥2,730,000)
Fiscal Year 2007: ¥12,350,000 (Direct Cost: ¥9,500,000、Indirect Cost: ¥2,850,000)
|
Research Abstract |
To reveal the cosmic structure formation, realization of wide field and sensitive submillimeter wavelength observations of distant galaxy clusters and protogalaxies along the large scale structure is required. Therefore, development of a sensitive large array cryogenic detector utilizing superconducting transision edge sensor "TES bolometers" was conducted and the array detector was successfully readout by efficient multiplexing method.
|