Paper
18 December 2000 Feasibility study of a camera for the UV Italian Sky Surveyor (UVISS) on the International Space Station
Salvatore Scuderi, Giovanni Bonanno, Santo Catalano, Alessandro C. Lanzafame, Oberto Citterio, Paolo Conconi, Giovanni Pareschi, Michela C. Uslenghi, Roberto Stalio
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Abstract
We present a feasibility study of a wide field UV imaging camera for the UV Italian Sky Surveyor (UVISS) under study by the Italian Space Agency as possible payload externally attached on an Express Pallet to the International Space Station. The camera will operate in the range 950 - 2700 angstrom, it will have a 1 square degree field of view with an expected angular resolution of about 3' at best. Two layouts are considered: the first is a camera based on the use of transmittance filters to select the bandpass of interest while the second one is based on the use of multilayers mirrors to define the bandpasses of the filters. In both options the detectors used will be intensified CCDs with an appropriate choice of photocathodes. Finally, we present some simulations to evaluate the performances of the camera.
© (2000) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Salvatore Scuderi, Giovanni Bonanno, Santo Catalano, Alessandro C. Lanzafame, Oberto Citterio, Paolo Conconi, Giovanni Pareschi, Michela C. Uslenghi, and Roberto Stalio "Feasibility study of a camera for the UV Italian Sky Surveyor (UVISS) on the International Space Station", Proc. SPIE 4139, Instrumentation for UV/EUV Astronomy and Solar Missions, (18 December 2000); https://doi.org/10.1117/12.410525
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KEYWORDS
Cameras

Mirrors

Optical filters

Indium

Ultraviolet radiation

Multilayers

Reflectivity

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