Lawrence, J. S., Ashley, M. C. B. & Storey, J. W. V., 2013, Astrophysics from Antarctica, 288, 6 | View on ADS (2013IAUS..288....6L) | Access via DOI
Antarctic astronomical site-testing has been conducted using autonomous self-powered observatories for more than a decade (the AASTO at South Pole, the AASTINO at Dome C, and PLATO at Dome A/Dome F). More recently autonomous (PLATO) observatories have been developed and deployed to support small-scale scientific instruments, such as HEAT, a 0.6 m aperture terahertz telescope at Ridge A, and AST3, a 0.5 m optical telescope array at Dome A. This paper reviews the evolution of autonomous Antarctic astronomical observatories, and discusses the requirements and implications for observatories that will be needed for future larger-scale facilities.
This publication has been tagged as:
Hemisphere/Antarctic
Site/Dome A (Kunlun Station)
Site/Dome C (Concordia Station)
Site/Dome F (Dome Fuji)
Site/Ridge A
Site/South Pole
Type/Instrument design
Type/Review
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