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Mid- and Far-Infrared Astronomy and
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| April 17 (Monday) | |||||
| 9:00-9:15 | Opening Remarks | T. Matsumoto (ISAS, Japan) | |||
1. Science with Large-Aperture Cooled Telescopes | |||||
| 1.1. Formation of Stars and Planets | Chair : | M. Hayashi (NAOJ, Japan) | |||
| 9:15-9:40 | Exoplanet photometry and spectroscopy with HII/L2 | M. Tamura (NAOJ, Japan) | |||
| 9:40-10:05 | Star formation and the NGST | M. Robberto (STScI/ESA) | |||
| 1.2. Stars | Chair : | M. Hayashi (NAOJ, Japan) | |||
| 10:05-10:30 | High-resolution spectroscopy of evolved stars: from ISO to HII/L2 | I. Yamamura (ISAS, Japan) | |||
| 10:30-10:45 | *** Tea Break *** | ||||
| 1.3. Interstellar Medium | Chair : | T. de Graauw (SRON, Netherlands) | |||
| 10:45-11:10 | The Interstellar Medium in the Mid- and Far-Infrared | G. Serabyn (JPL, USA) | |||
| 11:10-11:35 | Evolution of dust in galaxies and HII/L2 | T. Onaka (U. Tokyo, Japan) | |||
| 11:35-12:00 | Observability of Hydrogen Molecules in Infrared Regions | H. Shibai (Nagoya U., Japan) | |||
| 12:00-13:30 | *** Lunch *** | ||||
| 1.4. ULIRG and AGN | Chair : | Y. Taniguchi (Tohoku U., Japan) | |||
| 13:30-13:55 | Infrared spectroscopy of ultraluminous and active galaxies | D. Lutz (MPE, Germany) | |||
| 13:55-14:20 | Infrared luminous galaxies | D. Sanders (U.Hawaii, USA) | |||
| 1.5. High-z Galaxies and Primeval Galaxies | Chair : | Y. Taniguchi (Tohoku U., Japan) | |||
| 14:20-14:45 | Mid-Far Infrared Spectral Evolution of Elliptical Galaxies and Clusters of Galaxies at High Redshifts | N. Arimoto (U.Tokyo, Japan) | |||
| 14:45-15:10 | Galaxy populations from some deep ISO surveys | S. Oliver (ICSTM, UK) | |||
| 15:10-16:10 | *** Poster Session *** | ||||
| 1.6. Infrared Background Radiation and Cosmology | Chair : | J. Mather(GSFC, USA) | |||
| 16:10-16:35 | Observations of the Infrared Extragalactic Background Light | T. Matsumoto (ISAS, Japan) | |||
| 16:35-17:00 | Cosmochemical Evolution | M. Harwit (USA) | |||
| 18:00-20:00 | *** Party *** | ||||
| April 18 (Tuesday) | |||||
2. Future Missions | |||||
| 2.1. Future Infrared Missions | Chair : | D. Sanders (U. Hawaii, USA) | |||
| 9:00- 9:25 | HII/L2 mission | T. Nakagawa (ISAS, Japan) | |||
| 9:25- 9:50 | NGST | J. Mather (GSFC, USA) | |||
| 9:50-10:15 | NASA's Stratospheric Observatory for Far-Infrared Astronomy (SOFIA) | Sean C. Casey (ARC, USA) | |||
| 10:15-10:30 | *** Tea Break *** | ||||
| Chair : | M. Keesler (ESA) | ||||
| 10:30-10:55 | FIRST Mission | G. Pilbratt (ESTEC, Netherlands) | |||
| 10:55-11:20 | Focal Plane Instruments of FIRST | T. de Graauw (SRON, Netherlands) | |||
| 11:20-11:45 | Concepts of future missions: SPECS and SPIRIT | J. Mather (GSFC, USA) | |||
| 11:45-13:00 | *** Lunch *** | ||||
| 13:00-13:30 | *** ISAS Tour (Astro-F MTM) *** | ||||
| 2.2. Related Projects at Different Wavelengths | Chair : | H. Shibai (Nagoya U., Japan) | |||
| 13:30-13:50 | The Subaru Telescope and HII/L2 Mission | M. Hayashi(NAOJ, Japan) | |||
| 13:50-14:10 | Large Aperture Ground-based telescope | T. Hawarden(JAC, USA), and T. de Graauw (SRON, Netherlands) | |||
| 14:10-14:30 | Large Millimeter and Submillimeter Array | R. Kawabe (NAOJ, Japan) | |||
3. Key Technical Issues | |||||
| 3.1. Lightweight Telescopes | Chair : | T. Onaka (U. Tokyo, Japan) | |||
| 14:30-14:55 | Proposed telescope system for HII/L2 | I. Mikami (MELCO, Japan) | |||
| 14:55-15:20 | Development of Lightweight Mirror Technology and the Next Generation Space Telescope (NGST) | D. Jacobson (GSFC, USA) | |||
| 15:20-15:35 | *** Tea Break *** | ||||
| 3.2. Cryogenics | Chair : | H. Murakami (ISAS, Japan) | |||
| 15:35-16:00 | Cryogenic system for HII/L2 | M. Murakami (Tsukuba U., Japan) | |||
| 16:00-16:25 | Cryocoolers in Space | S. Castles (GSFC, USA) | |||
4. Discussion |
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| 16:25-17:15 | International Collaboration for the Future | ||||
| Organizer: | M. Harwit | ||||
| Presenter: | T. Matsumoto, M. Kessler, J. Mather, and T. de Graauw | ||||
We prepare an overhead projector and a video projector. If you need other special equipment, please contact LOC as soon as possible.
We request all speakers to prepare their viewgraphs with large characters, since the screen is not so large. We recommend no more than 7 lines in one viewgraph.
Maximum size of one poster is 90cm (width) X 130cm. The entrance lobby near the conference room is allocated for the poster presentation, and all posters are to be displayed during the whole period of the workshop. A special session for the poster papers is scheduled at 15:10-16:10 on April 17. We expect that each author will stand by his/her poster for the explanation during this session.
Last modified on April 8, 2000
h2l2_ws@koala.astro.isas.ac.jp