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Overview
| Title | The impact of near-infrared high-resolution spectroscopy on stellar physics |
| Date | 2016 October 5 (Wed) 9:30 ‐ 6 (Thu) 12:30 |
| Venue | Mukougaoka Faculty House (Seminar Room), The University of Tokyo (HP, map) |
Purpose
To discuss what we'll be able to do with near-IR spectroscopy in
the near future and what we should prepare for the transition from the optical to the IR.
Group Photo
Schedule
2016/10/05
| Time | Speaker | Title |
| 9:30-10:00 | N. Kobayashi | WINERED: overview (PDF) |
| 10:00-10:30 | M. Omiya | Infrared precise radial velocity survey of late-M dwarfs (PDF) |
| 10:30-11:00 | Break and free discussion |
| 11:00-11:30 | G. Bono | Science drivers for WINERED at NTT (PDF) |
| 11:30-12:00 | K. Fukue | Abundance determinations of Cepheids with NIR high-resolution spectroscopy (PDF) |
| 12:00-12:30 | C. Sneden (skype) | Highlights of the First Two Years of High-Resolution IGRINS H & K Band Observations (PDF) |
| 12:30-14:00 | Lunch |
| 14:00-14:30 | Y. Takeda | Near-IR stellar spectroscopy using Subaru/IRCS (PDF) |
| 14:30-14:40 | M. Hidai | WINERED spectra of metal-poor stars (PDF) |
| 14:40-15:10 | S. Hamano | The survey of near-infrared diffuse interstellar bands (PDF) |
| 15:10-15:40 | H. Sagawa | High dispersion spectra of CO2 in the Venus atmosphere obtained by WINERED (PDF) |
| 15:40-16:10 | H. Sameshima | Correction of WINERED WIDE-mode spectra for telluric absorption (PDF) |
| 16:10-16:15 | Group Photo |
| 16:15-16:40 | Break and free discussion |
| 16:40-17:10 | M. Nonino (skype) | Telluric lines correction via sky modelling (PDF) |
| 17:10-17:40 | N. Matsunaga | WINERED: atomic lines in late-type stars (PDF) |
| 17:40-18:10 | N. Przybilla | Non-LTE line-formation in the near-IR (PDF) |
| 18:30- | Banquet |
2016/10/06
| Time | Speaker | Title |
| 9:30-10:00 | C. Yasui | WINERED HIGH-RESOLUTION NEAR-INFRARED SPECTROSCOPY OF YOUNG INTERMEDIATE-MASS STARS: INSIGHTS INTO EVOLUTION OF STAR-DISK INTERACTIONS |
| 10:00-10:30 | M. Mizumoto | A Newly-identified Emission-line Region around P Cygni (PDF) |
| 10:30-11:00 | Break and free discussion |
| 11:00-11:30 | Y. Takagi | Estimating the evolution timescale of pre-main sequence stars and protoplanetary disks with high-resolution NIR spectroscopy (PDF) |
| 11:30-12:00 | T. Nakagawa | High-resolution spectroscopy of ISM toward galactic nuclei: synergy with circum-stellar material studies (PDF) |
| 12:00-12:30 | Discussion (Chair: G. Bono) |
Participants
| Name | Institute |
| Wako Aoki | National Astronomical Observatory of Japan |
| Giuseppe Bono | University of Rome Tor Vergata |
| Ryosuke Doi | ISAS/JAXA |
| Scarlet Saez Elgueta | The University of Tokyo |
| Masayuki Fujimoto | Hokkaido University/Hokkai Gakuen University |
| Kei Fukue | Kyoto Sangyo University |
| Satoshi Hamano | Kyoto Sangyo University |
| Masahide Hidai | Tokai University |
| Hiroyuki Ishikawa | GUAS, National Astronomical Observatory of Japan |
| Masato Ishizuka | The University of Tokyo |
| Mingjie Jian | The University of Tokyo |
| Naoto Kobayashi | The University of Tokyo |
| Jungmi Kwon | ISAS/JAXA |
| Hiroshi Maeshima | The University of Tokyo |
| Noriyuki Matsunaga | The University of Tokyo |
| Misaki Mizumoto | ISAS/JAXA, The University of Tokyo |
| Tadafumi Matsuno | GUAS, National Astronomical Observatory of Japan |
| Takao Nakagawa | ISAS/JAXA |
| Shogo Nishiyama | Miyagi University of Education |
| Mario Nonino (skype) | Astronomical Observatory of Trieste |
| Masashi Omiya | National Astronomical Observatory of Japan |
| Nobert Przybilla | University of Innsbruck |
| Hideo Sagawa | Kyoto Sangyo University |
| Hiroaki Sameshima | Kyoto Sangyo University |
| Takuma Suda | The University of Tokyo |
| Chris Sneden (skype) | The University of Texas at Austin |
| Yuhei Takagi | National Astronomical Observatory of Japan |
| Yoichi Takeda | National Astronomical Observatory of Japan |
| Chikako Yasui | National Astronomical Observatory of Japan |
Organizers
- Noriyuki Matsunaga (DoA, UTokyo)
- Takuji Tsujimoto (NAOJ)
- Naoto Kobayashi (IoA, UTokyo)
- Kei Fukue (Kohyama observatory and LiH, Kyoto Sangyo Univ)
- Sohei Kondo (Kohyama observatory and LiH, Kyoto Sangyo Univ)
- Giuseppe Bono (Univ Rome Tor Vergata)
Acknowledgements
This workshop is supported by NAOJ and Kakenhi (No. 26287028).