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Astrometric data for NEAs extracted from the infrared DENIS survey

Published online by Cambridge University Press:  01 October 2007

W. Thuillot ,
J. Berthier ,
J. Iglésias ,
G. Simon  and
V. Lainey
W. Thuillot
Affiliation:
Institut de mécanique céleste et de calcul des éphémérides, IMCCE-Paris Observatory 77, av. Denfert Rochereau, 75014, Paris, France email: [email protected]
J. Berthier
Affiliation:
Institut de mécanique céleste et de calcul des éphémérides, IMCCE-Paris Observatory 77, av. Denfert Rochereau, 75014, Paris, France email: [email protected]
J. Iglésias
Affiliation:
Institut de mécanique céleste et de calcul des éphémérides, IMCCE-Paris Observatory 77, av. Denfert Rochereau, 75014, Paris, France email: [email protected]
G. Simon
Affiliation:
GEPI, Paris Observatory 61 av. de l'Observatoire, Paris, France email: [email protected]
V. Lainey
Affiliation:
Institut de mécanique céleste et de calcul des éphémérides, IMCCE-Paris Observatory 77, av. Denfert Rochereau, 75014, Paris, France email: [email protected]
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Abstract

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When astrometric data can be extracted from archives, this generally allows us to get very strong constraints for the orbital modeling of Solar System objects. This is particularly important for Near-Earth Asteroids. We have developed tools in the Virtual Observatory framework in order to carry out such a task. We have applied them to the DENIS survey. This survey has been performed from 1995 to 2001 in the I, J, K' spectral bands with a 1m telescope at ESO La Silla. Many sources associated to Solar System Objects have been identified and we present our preliminary results.

Keywords

astrometrysurveysasteroids
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. 544 - 547
Copyright
Copyright © International Astronomical Union 2008