Optical Observing Conditions at Delingha Station

J.F. Tian, L.C. Deng, X.B. Zhang, X.M. Lu, J.J. Sun, Q.L. Liu, Q. Zhou, Z.Z. Yan, Y. Xin, K. Wang, X.J. Jiang, Z.Q. Luo, J. Yang
(Submitted on 2 Feb 2016)

SONG is a global ground based network of 1 meter telescopes for stellar time-domain science, an international collaboration involving many countries across the world. In order to enable a favourable duty cycle, the SONG network plans to create a homogeneous distribution of 4 nodes in each of the northern and southern hemispheres. A natural possibility was building one of the northern nodes in East Asia, preferably on the Qinghai-Tibetan Plateau. During the last decade, a great deal of effort has been invested in searching for high a quality site for ground based astronomy in China, since this has been one of the major concerns for the development of Chinese astronomy. A number of sites on the plateau have been in operation for many years, but most of them are used only for radio astronomy, as well as small optical telescopes for applied astronomy. Several potential sites for large optical instruments have been identified by the plateau site survey, but as yet none of them have been adequately quantitatively characterised. Here we present results from a detailed multi-year study of the Delingha site, which was eventually selected for the SONG-China node. We also describe the site monitoring system that will allow an isolated SONG and 50BiN node to operate safely in an automated mode.

Comments: 30 pages, 15 figures
Subjects: Instrumentation and Methods for Astrophysics (astro-ph.IM)
Cite as: arXiv:1602.00838 [astro-ph.IM] (or arXiv:1602.00838v1 [astro-ph.IM] for this version)
Submission history
From: Licai Deng
[v1] Tue, 2 Feb 2016 09:13:03 GMT (1211kb,D)
http://arxiv.org/abs/1602.00838