Hostname: page-component-78c5997874-94fs2 Total loading time: 0 Render date: 2024-11-17T21:27:43.110Z Has data issue: false hasContentIssue false
  • English
  • Français

JASMINE data analysis

Published online by Cambridge University Press:  01 October 2007

Y. Yamada ,
N. Gouda ,
T. Yano ,
Y. Kobayashi  and
Y. Niwa
Y. Yamada
Affiliation:
Department of Physics, Kyoto University, Oiwake-cho Kita-Shirakawa Kyoto 606-8502JAPAN email: yamada@amesh.org
N. 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
T. 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
Y. 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
Y. 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 UniversityKyoto 606-8501, JAPAN email: kazin.niwa@nao.ac.jp
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Japan Astrometry Satellite Mission for Infrared Exploration (JASMINE) aims to construct a map of the Galactic bulge with a 10 μas accuracy. We use z-band CCD or K-band array detector to avoid dust absorption, and observe about 10 × 20 degrees area around the Galactic bulge region.

In this poster, we show the observation strategy, reduction scheme, and error budget. We also show the basic design of the software for the end-to-end simulation of JASMINE, named JASMINE Simulator.

Keywords

methods: data analysis
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 3 , Symposium S248: A Giant Step: from Milli- to Micro-arcsecond Astrometry , October 2007 , pp. 407 - 408
Copyright
Copyright © International Astronomical Union 2008

References

Eichhorn, H., & Clary, W. G. 1974, MNRAS, 166, 425CrossRefGoogle 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
Zacharias, N., de Vegt, C., Nicholson, W., & Penston, M. J.CPC2 - the Second Cape Photographic Catalog II. Conventional plate adjustment and catalog construction. 1992 A&A 254, 397Google Scholar