| Budget Amount *help |
¥36,660,000 (Direct Cost: ¥28,200,000、Indirect Cost: ¥8,460,000)
Fiscal Year 2022: ¥1,690,000 (Direct Cost: ¥1,300,000、Indirect Cost: ¥390,000)
Fiscal Year 2021: ¥1,430,000 (Direct Cost: ¥1,100,000、Indirect Cost: ¥330,000)
Fiscal Year 2020: ¥2,860,000 (Direct Cost: ¥2,200,000、Indirect Cost: ¥660,000)
Fiscal Year 2019: ¥3,900,000 (Direct Cost: ¥3,000,000、Indirect Cost: ¥900,000)
Fiscal Year 2018: ¥26,780,000 (Direct Cost: ¥20,600,000、Indirect Cost: ¥6,180,000)
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| Outline of Final Research Achievements |
A new THz receiver with SIS mixers employing high critical current density junctions was installed on the ASTE telescope. Wide-field images were successfully obtained toward one of the nearest star-forming regions. THz observation capability on a 10 m-class single dish telescope in South America was established. Due to the global pandemic, high transition CO observation data were not obtained with ASTE. However, observations of nearby U/LIRGs using the ALMA telescope and other telescopes showed that dense gas and star formation/AGN activities were seen in these colliding galaxy systems. Furthermore, using the ALMA/ACA telescope, a correlation between carbon monoxide and neutral carbon was confirmed.
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