Abstract
Schemes using optical fibers to connect instruments to telescopes have been espoused ever since potentially useful fibers became available about a decade ago. The first published such use of fibers was apparently at Steward Observatory (HUBBARD, ANGEL and GRESHAM [1]). Since then, fiber-fed instrumentation has been constructed at numerous institutions (GRAY [2]; LUND and ENARD [3]; HILL, ANGEL and SCOTT [4], to name just a few). Theory and measurements have also been published dealing with the behavior of astronomically useful fibers (BARDEN, RAMSEY and TRUAX [5]; HJND [6]; HEACOX [7]; POWELL [8], and others).
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Ingerson, T.E. (1988). Fiber-Fed Instrumentation at CTIO. In: Robinson, L.B. (eds) Instrumentation for Ground-Based Optical Astronomy. Santa Cruz Summer Workshops in Astronomy and Astrophysics. Springer, New York, NY. https://doi.org/10.1007/978-1-4612-3880-5_21
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DOI: https://doi.org/10.1007/978-1-4612-3880-5_21
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