Poster + Paper
29 August 2022 Ground-based support of the planned WSO-UV mission
Author Affiliations +
Conference Poster
Abstract
Observational data in the ultraviolet wavelength region of the electromagnetic spectrum (120-300 nm) are a powerful tool for studying many astrophysical objects such as exoplanets, especially for determining the characteristics of their atmospheres. Numerous publications on exoplanetary research in leading astronomical publications, prepared in recent years on the basis of realized applications for observations on the instruments of the Hubble Space Telescope (HST), which is the main telescope for spectroscopy in UV, indicates its high demand by the astronomical community. Work is underway to create an orbital space observatory "Spektr-UF" (World Space Observatory - Ultraviolet), which will be the successor of the HST. The Institute of Astronomy RAS is the Lead scientific organization for this project and University Complutense of Madrid is the main WSO-UV partner. Within the framework of this research, work is planned to determine the characteristics for creating instruments for ground-based mission support, to develop tools for preparing applications for the observation program, to develop a program for scientific research of the project. In this paper we discuss spectroscopic and imaging instrumentations of Russian telescopes to be used as project ground support.
© (2022) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
M. Sachkov, S. Sichevsky, and Ana Inés Gómez de Castro "Ground-based support of the planned WSO-UV mission", Proc. SPIE 12184, Ground-based and Airborne Instrumentation for Astronomy IX, 121845R (29 August 2022); https://doi.org/10.1117/12.2629622
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KEYWORDS
Spectrographs

Telescopes

Ultraviolet radiation

Spectral resolution

Spectroscopes

Astronomy

Imaging spectroscopy

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