Control and monitoring software for the Greenland Telescope

被引：4
|
作者：
Patel, Nimesh A. [1 ]
Nishioka, Hiroaki [2 ]
Huang, Chih-Wei Locutus [2 ]
机构：
[1] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA
[2] Acad Sinica, Inst Astron & Astrophys, POB 23-141, Taipei, Taiwan
来源：
SOFTWARE AND CYBERINFRASTRUCTURE FOR ASTRONOMY IV | 2016年 / 9913卷
关键词：
Radio telescopes; Control software; Pointing calibration;
D O I：
10.1117/12.2232409
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The Greenland Telescope (GLT) is a 12m diameter antenna that is being developed from the ALMA North America prototype antenna, for VLBI observations and single-dish science approaching THz, at the Summit station in Greenland. The GLT is a collaboration between the Smithsonian Astrophysical Observatory and the Academia Sinica Institute of Astronomy and Astrophysics. We describe the control and monitoring software that is being developed for GLT. The present version of the software is ready for the initial tests of the antenna at Thule, including optical and radio pointing calibration, holography, and VLBI observations at 230 GHz.
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页数：8
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