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Time-domain survey of the Galactic anti-center using Nanshan 1m telescope

Published online by Cambridge University Press:  27 October 2016

T.-Z. Yang ,
A. Esamdin ,
J.-N. Fu ,
L. Ma ,
J.-Z. Liu  and
F.-F. Song
T.-Z. Yang
Affiliation:
Xinjiang Astronomical Observatory, CAS, Urumqi, Xinjiang, China email: aliyi@xao.ac.cn University of Chinese Academy of Sciences, Beijing, China email: yangtaozhi@xao.ac.cn
A. Esamdin
Affiliation:
Xinjiang Astronomical Observatory, CAS, Urumqi, Xinjiang, China email: aliyi@xao.ac.cn
J.-N. Fu
Affiliation:
Department of Astronomy, Beijing Normal University, Beijing, China
L. Ma
Affiliation:
Xinjiang Astronomical Observatory, CAS, Urumqi, Xinjiang, China email: aliyi@xao.ac.cn
J.-Z. Liu
Affiliation:
Xinjiang Astronomical Observatory, CAS, Urumqi, Xinjiang, China email: aliyi@xao.ac.cn
F.-F. Song
Affiliation:
Xinjiang Astronomical Observatory, CAS, Urumqi, Xinjiang, China email: aliyi@xao.ac.cn University of Chinese Academy of Sciences, Beijing, China email: yangtaozhi@xao.ac.cn
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Abstract

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Following the LAMOST Spectroscopic Survey and Xuyi's Photometric Survey of the Galactic anti-center (GAC), we plan to conduct a time-domain survey of GAC to study the variable sky using Nanshan 1m telescope. The survey will be conducted during winter (in Nov., Dec., and Jan.). The first goal of the survey is to cover 270 sq.deg. of sky area in three years. The survey intends to detect some strong transient events of stars and find some short time-scale variable stars of different types. In this paper, we introduce the survey and present the preliminary results already carried out.

Keywords

surveystechniques: photometricstars: binariesoscillations
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 11 , General Assembly A29B: Astronomy in Focus , August 2015 , pp. 517 - 520
Copyright
Copyright © International Astronomical Union 2016 

References

Boonyarak, C., Jing, S. Y., & Khokhuntod, P., Fu, J. N. 2011, Ap&SS, 125, 131 Google Scholar
Cui, X.-Q., Zhao, Y.-H., & Chu, Y.-Q., et al. 2012, RAA, 12, 1197 Google Scholar
Djorgovski, S. G., et al. 2011, IAU Symposium, 285, 2011 Google Scholar
Fu, J.-N., Zhang, C., & Marak, M., et al. 2008, ChjAA, 8, 237 Google Scholar
Liu, X.-W., et al. (2013), IAU Symposium, 298, 2013 Google Scholar
Ward, R., Delaney, P., & Sadavoy, S., et al. 2008, JRASC, 102, 134 Google Scholar
Wils, P., Kleidis, S., & Hambsch, F. J. 2009, IBVS, 5878, 2009Google Scholar
Yang, X. H., Fu, J. N., & Zha, Q. 2012, AJ, 144, 92 CrossRefGoogle Scholar
Zhao, G., Zhao, Y.-H., Chu, Y.-Q., Jing, Y.-P., & Deng, L.-C. 2012, RAA, 12, 723 Google Scholar
Zhang, H.-H., Liu, X.-W., Yuan, H.-B., et al. 2014, RAA, 14, 456 Google Scholar
Zhou, A. Y. 2006, Ap&SS, 301: 11–20 Google Scholar