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World space observatory-ultraviolet

Published online by Cambridge University Press:  11 June 2009

P. Kern ,
A. Shugarov ,
B. Shustov ,
M. Sachkov ,
A.I. Gomez de Castro ,
K. Werner ,
N. Kappelmann  and
M. Huang
A. Shugarov
Affiliation:
Institute of Astronomy, RAS, Russia
B. Shustov
Affiliation:
Institute of Astronomy, RAS, Russia
M. Sachkov
Affiliation:
Institute of Astronomy, RAS, Russia
A.I. Gomez de Castro
Affiliation:
Fac. de CC. Matematicas,Universidad Complutense de Madrid, Plaza de Ciencias 3, 28040 Madrid, Spain
K. Werner
Affiliation:
Institut fur Astronomie und Astrophysic, Abteilung Astronomie (IAAT), Universitat Tubingen, Tubingen, 72076, Germany
N. Kappelmann
Affiliation:
Institut fur Astronomie und Astrophysic, Abteilung Astronomie (IAAT), Universitat Tubingen, Tubingen, 72076, Germany
M. Huang
Affiliation:
National Astronomical Observatories, CAS, China
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Abstract

The World Space Observatory UltraViolet (WSO-UV) project is aninternational space observatory designed for observations in theultraviolet domain. The observatory includes a single 170 cmaperture telescope capable of high-resolution spectroscopy, longslit low-resolution spectroscopy and deep UV and optical imaging.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 37: Astrophysics Detector Workshop 2008 , 2009 , pp. 217 - 222
Copyright
© EAS, EDP Sciences, 2009

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References

Barnstedt, J., et al., 1999, A&AS, 134, 561
Gomez de Castro, A.I., Pagano, I., Sachkov, M., et al., 2007, Stellar Populations II, ed. M. Chavez, Proc. of the conference held in Puerto Vallarta, Mexico
Kappelmann, N., Barnstedt, J., Gringel, W., et al., 2006, Space Telescopes and Instrumentation II: Ultraviolet to Gamma Ray, ed. Turner Martin J.L. & Hasinger G., Proc. SPIE, 6266, 62660X CrossRef
Sanko, N., & Shustov, B., 2006, Space physics, ed. P.E. Zakharova, Proc. Conf. Held Ekaterinburg, Russia, XXXV