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Preliminary Results of Low Dispersion Asteroid Spectroscopy Survey at NAO Rozhen

Published online by Cambridge University Press:  07 March 2018

Elena Vchkova Bebekovska
Affiliation:
Institute of Physics, Faculty of Natural Sciences and Mathematics, University Ss. Cyril and Methodius, Skopje, Republic of Macedonia email: [email protected]
Galin Borisov
Affiliation:
Armagh Observatory, College Hill, BT61 9DG Armagh, Northern Ireland, UK email: [email protected] Institute of Astronomy and National Astronomical Observatory, Bulgarian Academy of Sciences
Zahary Donchev
Affiliation:
Institute of Astronomy and National Astronomical Observatory, Bulgarian Academy of Sciences
Gordana Apostolovska
Affiliation:
Institute of Physics, Faculty of Natural Sciences and Mathematics, University Ss. Cyril and Methodius, Skopje, Republic of Macedonia email: [email protected]
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Abstract

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We are presenting the first results of low dispersion spectroscopic observation of asteroids at Bulgarian National Astronomical Observatory Rozhen. Asteroids with unclassified spectra and brighter than 15 magnitude have been chosen. Besides just presenting the asteroid reflectance, classification according to Bus S. J. et al. (2012) has been done. The asteroid spectra of 590 Tomyris, 703 Noemi, 1596 Itzigsohn and 1826 Miller are presented together with standard spectra corresponding to the three best matches given by the public software tool M4AST (Popescu M. et al. (2012)). Our aim is to participate in the coordinated program of asteroids spectroscopy complementary to the observations of Gaia.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2018 

References

Bus, S. J., Vilas, F. & Barucci, M. A. 2012, Asteroids III, Univ. of Arizona Press, 169-182.Google Scholar
Jockers, K. et al. 2000, Kinematika i Fizika Neb. Tel. Suppl., 3, 13 Google Scholar
Popescu, M. et al. 2012, Astronomy & Astrophysics, 544, A130 Google Scholar