The 1st miniTAO/ANIR Science Workshop on 9 April, 2010
The near-infrared camera, ANIR, mounted on the University of Tokyo miniTAO 1-m telescope has begun scientific observations last year, becoming successful in detecting the Hydrogen Emission Line from the Galactic Center in the Infrared Light.
We have held the 1st science workshop on 9 April in order to keep carrying out observations in various astronomical fields, where we have reported/discussed the progress of the data analysis and astronomical targets to be observed in the future.
| |
▲ Participants in Mitaka
|
| Date： | April 9 (Fri), 2010 10:00-17:00 |
| Venue： | Institute of Astronomy, the University of Tokyo (Mitaka) |
| Program： | Reports |
| 10:00-10:15 | The current status of ANIR | Konishi |
| 10:15-10:30 | ANIR Paschen alpha surveys | Motohara |
| 10:30-10:50 | Paαobservations of SMC cluster NGC330 | Tanabe |
| 10:50-11:10 | Detection of H2O absorption (1.9µm Ω-band) from a late M star | Tanabe |
| 11:10-11:30 | H2O Molecular absorption in Mira-type variable stars | Matsunaga |
| 13:00-13:30 | 1. Multi-band monitoring observations of hypernovae, 2. X-ray, optical and NIR monitoring observations of Seyfert galaxies | Minezaki |
| 13:30-13:50 | MSAGN (Mid-Infrared Search for Active Galactic Nuclei) | Oyabu |
| Proposal |
| 14:00-14:20 | Survey of YSO Eclipsing Binaries in star-forming regions | Yamashita |
| 14:20-14:40 | Search for Wolf-Rayet stars as a host object for core-collapse massive supernovae | Tanaka |
| 14:40-15:00 | Obscured star formation in interacting galaxies | Komugi |
| 15:00-15:20 | Upper limit on star formation rate density due to collision of galaxies | Takagi |
| 15:20-15:35 | ANIR observation of transit planets near M dwarf stars | Narita |
| Data Analysis and Discussion |
| 15:40-16:00 | ANIR Data Reduction | Motohara |
| 16:00-17:00 | Discussion | Motohara |
|
|
