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Nano-JASMINE: use of AGIS for the next astrometricsatellite

Published online by Cambridge University Press:  15 February 2011

C. Turon ,
F. Meynadier ,
F. Arenou ,
Y. Yamada ,
N. Gouda  and
U. Lammers
Y. Yamada
Affiliation:
Department of Physics, Kyoto University, Oiwake-cho Kita-Shirakawa, Kyoto 606-8502, Japan. e-mail: [email protected]
N. Gouda
Affiliation:
JASMINE project office, National Astronomical Observatory JAPAN, Osawa Mitaka Tokyo, 181-8588, Japan
U. Lammers
Affiliation:
European Space Astronomy Center, European Space Agency, Madrid, Spain
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Abstract

The core data reduction for the Nano-JASMINE mission is planned to be done with Gaia’sAstrometric Global Iterative Solution (AGIS). The collaboration started at 2007 promptedby Uwe Lammers’ proposal. In addition to similar design and operating principles of thetwo missions, this is possible thanks to the encapsulation of all Gaia-specific aspects ofAGIS in a Parameter Database. Nano-JASMINE will be the test bench for Gaia AGIS software.We present this idea in detail and the necessary practical steps to make AGIS work withNano-JASMINE data. We also show the key mission parameters, goals, and status of the datareduction for the Nano-JASMINE.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 45: GAIA: At the Frontiers of Astrometry , 2010 , pp. 135 - 140
Copyright
© EAS, EDP Sciences 2011

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References

Références

Mignard, F., 2003, Gaia Spectroscopy, Science and Technology, ASP Conf. Ser., 298, 25
O’Mullane, W., & Lammers, U., 2008, GAIA-CZ-TN-ESAC-WOM-026-1
Lammers, U., 2010, GAIA-CZ-MN-ESAC-UL-043-01
Yamada, Y., 2010, GAIA-CZ-TN-KU-YY-001-01
Michalik, D., 2010, GAIA-CZ-ICD-ESAC-MIC-001-1
Gouda, N., 2010, in these proceedings
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