Abstract
Optical fibres have revolutionised observational astronomy over the past 17 years through the technique of multi-object spectroscopy. Ever since they were first used in 1979 at Steward Observatory (Hill et al. 1980) many observatories have built and used multi-fibre spectrographs because they are vital for many branches of astronomy requiring large spectroscopic samples. This paper reviews the use of optical fibres for multi-object spectroscopy in astronomy including a survey of multi-fibre facilities. A few important examples of scientific research carried out with multi-fibre spectrographs are also given and the future prospects for the technique are discussed. The uses of fibres for other astronomical applications such as high-precision radial velocity work or interferometry are not discussed.
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Parry, I.R. (1997). Multi-Object Spectroscopy with Optical Fibres. In: Kontizas, E., Kontizas, M., Morgan, D.H., Vettolani, G.P. (eds) Wide-Field Spectroscopy. Astrophysics and Space Science Library, vol 212. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-5722-3_1
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DOI: https://doi.org/10.1007/978-94-011-5722-3_1
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