| Budget Amount *help |
¥30,550,000 (Direct Cost: ¥23,500,000、Indirect Cost: ¥7,050,000)
Fiscal Year 2012: ¥6,500,000 (Direct Cost: ¥5,000,000、Indirect Cost: ¥1,500,000)
Fiscal Year 2011: ¥9,490,000 (Direct Cost: ¥7,300,000、Indirect Cost: ¥2,190,000)
Fiscal Year 2010: ¥14,560,000 (Direct Cost: ¥11,200,000、Indirect Cost: ¥3,360,000)
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| Research Abstract |
To realize wide field of view (FoV) and high sensitive observations in the millimeter wavelengths to terahertz, superconducting detector array has been developed. To investigate galaxy formation after the big-bang, submillimeter observations are extremely important. With our heritage of low noise ALMA superconducting detector developments, we demonstrated 500 pixel submillimeter camera with NEP of 6x10^<-18> W/rHz at low temperature of 0.1 K.
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