| Budget Amount *help |
¥191,620,000 (Direct Cost: ¥147,400,000、Indirect Cost: ¥44,220,000)
Fiscal Year 2022: ¥27,300,000 (Direct Cost: ¥21,000,000、Indirect Cost: ¥6,300,000)
Fiscal Year 2021: ¥26,390,000 (Direct Cost: ¥20,300,000、Indirect Cost: ¥6,090,000)
Fiscal Year 2020: ¥29,640,000 (Direct Cost: ¥22,800,000、Indirect Cost: ¥6,840,000)
Fiscal Year 2019: ¥62,010,000 (Direct Cost: ¥47,700,000、Indirect Cost: ¥14,310,000)
Fiscal Year 2018: ¥46,280,000 (Direct Cost: ¥35,600,000、Indirect Cost: ¥10,680,000)
|
|---|
| Outline of Final Research Achievements |
We operate the Tomo-e Gozen camera on the Kiso Schmidt telescope, and observed many SNe including a SNIa with early luminosity enhancement. We develop a three-band optical imager TriCCS for the Seimei telescope, and have observed SNe. TriCCS is also used for open use programs. NIR spectrograph NICE for the TAO telescope is updated for the use of very high altitude. We showed that observational properties of a luminous SNIa with early luminosity enhancement can be explained well by Carbon rich outer layers. We also showed that incomplete explosion of a white dwarf can explain many properties of a subluminous SNIa. We also worked for diversity of SNeIa and for other transients.
|
| Assessment Rating |
Ex-post Assessment Comments (Rating)
A: In light of the aim of introducing the research area into the research categories, expected outcomes of research have been produced.
|
Assessment Rating |
Interim Assessment Comments (Rating)
A: In light of the aim of introducing the research area into the research categories, the expected progress has been made in research.
|
