| Budget Amount *help |
¥18,200,000 (Direct Cost: ¥14,000,000、Indirect Cost: ¥4,200,000)
Fiscal Year 2013: ¥780,000 (Direct Cost: ¥600,000、Indirect Cost: ¥180,000)
Fiscal Year 2012: ¥4,680,000 (Direct Cost: ¥3,600,000、Indirect Cost: ¥1,080,000)
Fiscal Year 2011: ¥12,740,000 (Direct Cost: ¥9,800,000、Indirect Cost: ¥2,940,000)
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| Research Abstract |
We carried out studies to constrain the progenitor mass of the core collapse supernovae by studying the explosion site of nearby supernovae with optical IFU, narrow-band imaging, and other observations.
We published two papers in which we constrain mass and metalicity of the nearby core collapse supernovae using the data taken with SNIFS on UH88inch telescope and with GMOS on GEMINI-N telescope. We also develop a new instrument LISS (Line Imager and Slit Spectrograph) with which we can carry out narrow-band imaging with a Fabry-Perot etalon.
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