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SWIMS Science Workshop was held

The second science workshop for the near-infrared multi-object spectrograph SWIMS currently under development for the TAO 6.5 m telescope was held since the first one in 2009. In the meantime, as the instrument performance is being evaluated, a variety of specific observation proposals were presented. In the future, SWIMS will go through the comprehensive performance evaluation test at Mitaka and will be installed onto the Subaru Telescope of the NAOJ Hawaii Observatory to conduct the actual performance evaluation tests and early science observations in 2015. It will be then transported to Chile to see its first light on the TAO 6.5 m telescope in FY2017.

workshop discussion
Participants of the workshop Discussions among participants

In this workshop, with a view to actual observation, there were many specific observation proposals on such as cosmology, distant / nearby galaxies, AGNs, supernovae and galactic objects, including six invited talks. Those are so practical that can fully exploit the performance of the site and the instrument; the atmosphere at the high-altitude site is transparent in almost all the near-infrared wavelengths due to high altitude, and the instrument is capable of wide-field imaging, multi-object spectroscopy, and integral-field spectroscopy. We had high expectations for SWIMS from the presentations. In total, 40 people participated including those who via telecon.

Date August 5, 2013 Fri. 9:30-18:20
Venue: Lecture room, Institute of Astronomy, University of Tokyo
Program: Time Speaker Title
9:30-9:40 K. Motohara *1 Current status and schedule of TAO/SWIMS
9:40-9:55 M. Konishi *1 SWIMS overview
9:55-10:02 S. Nishijima *1 Detector
10:02-10:09 K. Tateuchi *1 Filter
10:09-10:16 H. Takahashi *1 MOS unit
10:16-10:23 Y. Kitagawa *1 IFU
[Cosmology]
10:30-11:00 T. Totani*2 (Invited Talk) From FastSound to SWIMS?
11:00-11:18 T. Minezaki*1 Measurement of luminosity distances of high-redshift quasars
[High-z galaxy]
11:18-11:48 T. Kodama*3 (Invited Talk) SWIMS18 Survey to explore the high-noon of galaxy formation
13:00-13:18 K. Tadaki*3 Resolving galaxies by SWIMS + WFC3
13:18-13:36 I. Tanaka*3 "Green Beans" Survey of proto-clusters of galaxies @ z=3.2-3.6 by [OIII] emitters
[AGN]
13:36-14:06 T. Nagao*4 (Invited Talk) Broad-band near-infrared spectroscopic observation of high-redshift active galactic nuclei
14:06-14:24 H. Sameshima*5 Chemical evolution of ionized gas in active galactic nuclei revealed with SWIMS
[Nearby galaxy]
14:40-15:10 S. Komugi*3 (Invited Talk) A study of galactic and extra-galactic star formation connected with SWIMS and ALMA
15:10-15:28 T. Saito*3 Star formation of nearby merging galaxies by spectroscopic observation of SWIMS and ALMA
15:28-15:46 K. Tateuchi*1 Elucidation of morphological formation of nearby galaxies using SWIMS / NBF&IFU
[Supernovae]
15:46-16:16 K. Maeda*6 (Invited Talk) Supernovae Science in Near-Infrared region
[Galactic objects]
16:16-16:46 N. Matsunaga*2 (Invited Talk) Toward establishing Mira-type variable stars as distance ladder / population indicator
16:46-17:04 K. Ebisawa*5 On the origin of the Galactic ridge X-ray radiation
17:04-17:22 H. Takahashi*1 Elucidation of constituent elements and evolution process of massive star clusters explored by SWIMS
17:22-17:40 K. Fukui*3 Observation of atmosphere of Transiting exoplanets using SWIMS
[Discussion]
17:50-18:20 Future directions etc.
Regarding affiliation of speaker
*1: Institute of Astronomy, Graduate School of Science, the University of Tokyo
*2: Department of Astronomy, Graduate School of Science, the University of Tokyo
*3: National Astronomical Observatory of Japan
*4: Kyoto University
*5: Japan Aerospace Exploration Agency
*6: Kavli Institute for the Physics and Mathematics of the Universe

Between the talks, we have demonstrated the operation of the multi-object spectroscopy unit, which is currently under performance evaluation tests at the laboratory building. Participants showed strong interest in the actual motion of the mask exchange.

workshop

Participants observing the MOSU demonstration

For further information on SWIMS, please refer to the following.