Design of a Wide Spectral Range and High-Resolution Spectrograph for Monitoring the Night Sky Background for Use in Air Fluorescence Telescopes

Physics – Medical Physics

Scientific paper

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Scientific paper

In this work we present the design of a compact, high-resolution echelle spectrograph for monitoring the Night Sky Background. This spectrograph is combined with a 25.4 cm telescope and uses an appropriate CCD camera as detector. It can operate in a wide spectral range from Ultraviolet to near Infrared (i.e. 300-780 nm) corresponding to the sensitivity spectral window of photocathodes used in the fluorescence telescopes. In the design we also made effort to compromise a sufficient sensitivity and a reasonable exposure time. This instrumentation could become a versatile tool for the operation and development of fluorescence telescopes used in Ultra High Energy Cosmic Ray Experiments.

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