Imaging, Spectroscopic, High-Contrast, and Interferometric Instrumentation

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

[+] Author Affiliations
Pablo Marcos-Arenal, Ana I. Gómez de Castro, Belén Perea Abarca

Universidad Complutense de Madrid, AEGORA Research Group, Spain

Mikhail Sachkov

Institute of Astronomy RAS, Moscow, Russia

J. Astron. Telesc. Instrum. Syst. 3(2), 025002 (Jun 05, 2017). doi:10.1117/1.JATIS.3.2.025002
History: Received October 5, 2016; Accepted May 11, 2017
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Abstract.  The World Space Observatory Ultraviolet telescope is equipped with high dispersion (55,000) spectrographs working in the 1150 to 3100 Å 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.

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© 2017 Society of Photo-Optical Instrumentation Engineers

Citation

Pablo Marcos-Arenal ; Ana I. Gómez de Castro ; Belén Perea Abarca and Mikhail Sachkov
"WUVS simulator: detectability of spectral lines with the WSO-UV spectrographs", J. Astron. Telesc. Instrum. Syst. 3(2), 025002 (Jun 05, 2017). ; http://dx.doi.org/10.1117/1.JATIS.3.2.025002


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