Testing and Data Reduction of the Chinese Small Telescope Array (CSTAR) for Dome A, Antarctica
arXiv:1001.4935 · doi:10.1088/1674-4527/10/3/009
Abstract
The Chinese Small Telescope ARray (hereinafter CSTAR) is the first Chinese astronomical instrument on the Antarctic ice cap. The low temperature and low pressure testing of the data acquisition system was carried out in a laboratory refrigerator and on the 4500m Pamirs high plateau, respectively. The results from the final four nights of test observations demonstrated that CSTAR was ready for operation at Dome A, Antarctica. In this paper we present a description of CSTAR and the performance derived from the test observations.
Accepted Research in Astronomy and Astrophysics (RAA) 1 Latex file and 20 figures
References in corpus (2)
Cited by in corpus (10)
- Photometry of Variable Stars from Dome A, Antarctica: Results from the 2010 Observing Season
- Photometry of Variable Stars from Dome A, Antarctica
- The First Release of the AST3-1 Point Source Catalogue from Dome A, Antarctica
- Variable Stars Observed in the Galactic Disk by AST3-1 from Dome A, Antarctica
- Stellar Variability and Flare Rates from Dome A, Antarctica using 2009 and 2010 CSTAR Observations
- Four winters of photometry with ASTEP South at Dome C, Antarctica
- Astronomy from Dome A in Antarctica
- Stellar Flares in the CSTAR Field: Results from the 2008 Data Set
- Automation of the AST3 optical sky survey from Dome~A, Antarctica
- ASTEP South: a first photometric analysis