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WUVS simulator: detectability of spectral lines with the WSO-UV spectrographs

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Marcos-Arenal, P. y Gómez de Castro, Ana Inés y Abarca, B. P. y Sachkov, Mikhail WUVS simulator: detectability of spectral lines with the WSO-UV spectrographs. Journal of Astronomical Telescopes, Instruments, and Systems, 3 (2). 025002-1. ISSN 2329-4124

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Resumen

The World Space Observatory Ultraviolet telescope is equipped with high dispersion (55,000) spectrographs working in the 1150 to 3100 angstrom spectral range. To evaluate the impact of the design on the scientific objectives of the mission, a simulation software tool has been developed. This simulator builds on the development made for the PLATO space mission and it is designed to generate synthetic time-series of images by including models of all important noise sources. We describe its design and performance. Moreover, its application to the detectability of important spectral features for star formation and exoplanetary research is addressed.


Tipo de documento:Artículo
Palabras clave:Space missions; Ultraviolet detector; Ultraviolet spectrograph; Simulations; CCD
Materias:Ciencias > Matemáticas > Lógica simbólica y matemática
Código ID:44797
Depositado:28 Sep 2017 08:09
Última Modificación:28 Sep 2017 10:27

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