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Nano-JASMINE: Simulation of Data Outputs

Published online by Cambridge University Press:  15 February 2011

C. Turon ,
F. Meynadier ,
F. Arenou ,
Y. Kobayashi ,
T. Yano ,
Y. Hatsutori ,
N. Gouda ,
J. Murooka ,
Y. Niwa  and
Y. Yamada
Y. Kobayashi
Affiliation:
National Astronomical Observatory, 2-21-1 Osawa Mitaka-shi, Tokyo, Japan
T. Yano
Affiliation:
National Astronomical Observatory, 2-21-1 Osawa Mitaka-shi, Tokyo, Japan
Y. Hatsutori
Affiliation:
National Astronomical Observatory, 2-21-1 Osawa Mitaka-shi, Tokyo, Japan
N. Gouda
Affiliation:
National Astronomical Observatory, 2-21-1 Osawa Mitaka-shi, Tokyo, Japan
J. Murooka
Affiliation:
The University of Tokyo, 7-3-1 Hongo Bunkyo-ku, Tokyo, Japan
Y. Niwa
Affiliation:
The University of Tokyo, 7-3-1 Hongo Bunkyo-ku, Tokyo, Japan
Y. Yamada
Affiliation:
Kyoto University, Kitashirakawa-oiwake-cho Sakyo-ku, Kyoto, Japan
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Abstract

We simulated the data outputs of the first Japanese astrometry satellite Nano-JASMINE, which is scheduled to be launched by the Cyclone-4 rocket in August 2011. The simulations were carried out using existing stellar catalogues such as the Hipparcos catalogue, the Tycho catalogue, and the Guide Star catalogue version 2.3. Several statics are shown such as the number of stars those will be measured distances using annual aberration observations. The method for determining the initial direction of the satellite’s spin axis has also been discussed. In this case, the frequency of bright stars observed by the satellite is an important factor.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 45: GAIA: At the Frontiers of Astrometry , 2010 , pp. 401 - 404
Copyright
© EAS, EDP Sciences 2011

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References

Références

Kobayashi, Y., et al., 2006, Proc. SPIE , 6265, 626544 CrossRef
Lasker, B.M., et al., 2008, AJ, 136, 735 CrossRef
Perryman, M.A.C., et al., 1997, A&A, 323, 49