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JASMINE – design and method of data reduction

Published online by Cambridge University Press:  01 July 2007

Yoshiyuki Yamada ,
Naoteru Gouda ,
Taihei Yano ,
Yukiyasu Kobayashi  and
Yoshito Niwa
Yoshiyuki Yamada
Affiliation:
Department of Physics, Kyoto University, Kyoto 606-8502, Japan email: yamada@amesh.org
Naoteru Gouda
Affiliation:
National Astronomical Observatory of Japan, National Institutes of Natural Sciences, Mitaka, Tokyo, 181-8588, Japan email: naoteru.gouda@nao.ac.jp, yuki@merope.mtk.nao.ac.jp, t.yano@nao.ac.jp
Taihei Yano
Affiliation:
National Astronomical Observatory of Japan, National Institutes of Natural Sciences, Mitaka, Tokyo, 181-8588, Japan email: naoteru.gouda@nao.ac.jp, yuki@merope.mtk.nao.ac.jp, t.yano@nao.ac.jp
Yukiyasu Kobayashi
Affiliation:
National Astronomical Observatory of Japan, National Institutes of Natural Sciences, Mitaka, Tokyo, 181-8588, Japan email: naoteru.gouda@nao.ac.jp, yuki@merope.mtk.nao.ac.jp, t.yano@nao.ac.jp
Yoshito Niwa
Affiliation:
National Astronomical Observatory of Japan, National Institutes of Natural Sciences, Mitaka, Tokyo, 181-8588, Japan email: naoteru.gouda@nao.ac.jp, yuki@merope.mtk.nao.ac.jp, t.yano@nao.ac.jp Graduate School of Human and Environment Study, Kyoto University, Kyoto 606-8501, Japan email: kazin.niwa@nao.ac.jp
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Abstract

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Japan Astrometry Satellite Mission for Infrared Exploration (JASMINE) aims to construct a map of the Galactic bulge with 10 μ arc sec accuracy. We use z-band CCD for avoiding dust absorption, and observe about 10 × 20 degrees area around the Galactic bulge region. Because the stellar density is very high, each FOVs can be combined with high accuracy. With 5 years observation, we will construct 10 μ arc sec accurate map.

In this poster, I will show the observation strategy, design of JASMINE hardware, reduction scheme, and error budget. We also construct simulation software named JASMINE Simulator. We also show the simulation results and design of software.

Keywords

astrometryinfrared:galaxies
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 3 , Symposium S245: Formation and Evolution of Galaxy Bulges , July 2007 , pp. 419 - 420
Copyright
Copyright © International Astronomical Union 2008

References

Yamada, Y., Gouda, N., Yano, T., Kobayashi, Y., Sako, N., & JASMINE Working Group 2007a, Advances in Space Research 40, 675CrossRefGoogle Scholar
Yamada, Y., Sako, N., Hatsutori, Y., Katagishi, H., Tanaka, T., Inamori, T., Yamauchi, M., Yano, T., & Gouda, N. 2007b, Report of the National Astronomical Observatory of JAPAN 10, 1Google Scholar
Kamata, Y., Miyazaki, S., Nakaya, H., Tsuru, T. G., Takagi, S., Tsunemi, H., Miyata, E., Muramatsu, M., Suzuki, H., & Miyaguchi, K. 2006, High Energy, Optical, and Infrared Detectors for Astronomy II. Edited by Dorn, David A.; Holland, Andrew D.. Proceedings of the SPIE, 6276, 62761U.Google Scholar