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Astrometry and Spectra Classification of Near Earth Asteroids with Lijiang 2.4m Telescope

Published online by Cambridge University Press:  07 March 2018

X. L. Zhang ,
B. Yang  and
J. M. Bai
X. L. Zhang
Affiliation:
Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011, China email: [email protected] Key Laboratory of the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming 650011, China
B. Yang
Affiliation:
Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011, China email: [email protected] Key Laboratory of the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming 650011, China
J. M. Bai
Affiliation:
Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011, China email: [email protected] Key Laboratory of the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming 650011, China
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Abstract

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The Lijiang 2.4m telescope of Yunnan Observatories is located at longitude E100°01′51″, latitude N26°42′32″ and height 3250m above sea level (IAU code O44). Because of low latitude of the site, long-focus system and planetary tracking mode of telescope, high accuracy positioning and spectral classification of the near Earth objects (NEAs) especially in the Southern Hemisphere can be studied with the Lijiang 2.4m telescope. As a set of observational campaigns organized by the GAIA-FUN-SSO, astrometry of several near Earth asteroids including (367943) Duende and (99942) Apophis were made with Lijiang 2.4m telescope during 2013. From December 12, 2015, spectra of three near earth asteroids were also observed with the YFOSC terminal attached to the Lijiang 2.4m telescope. This paper will give the detailed introduction of Lijiaing 2.4m telescope and observational results of near Earth asteroids obtained with it.

Keywords

methods: observationaltechniques: astrometryspectrum classification
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 12 , Symposium S330: Astrometry and Astrophysics in the Gaia sky , April 2017 , pp. 413 - 414
Copyright
Copyright © International Astronomical Union 2018 

References

Bus, S. J., Vilas, F., & Barucci, M. A. 2002, Asteroids III, 169Google Scholar
Thuillot, W., Bancelin, D., Ivantsov, A., et al. 2015, A&A, 583, A59 Google Scholar
Wang, N., Peng, Q. Y., Zhang, X. L., et al. 2015, MNRAS, 454, 3809 Google Scholar
Zhang, X. L., Yu, Y., Wang, X. L., et al. 2015, RAA, 15, 3, 170 Google Scholar