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A&A 414, L49-L52 (2004)
DOI: 10.1051/0004-6361:20031761
Letter
Detection of Saturnian X-ray emission with XMM-Newton
J.-U. Ness, J. H. M. M. Schmitt and J. RobradeHamburger Sternwarte, Universität Hamburg, Gojenbergsweg 112, 21029 Hamburg, Germany
(Received 5 December 2003 / Accepted 19 December 2003)
Abstract
The giant planet
Saturn was observed by XMM-Newton in September 2002. We present and analyse
these XMM-Newton observations and compare our findings to the Chandra
observations of Saturn. Contamination of the XMM-Newton data by optical light
is found to be severe in the medium and thin filters, but with the thick filter
all optical light is sufficiently blocked and the signal observed in this
filter is interpreted as genuine X-ray emission, which is found to
qualitatively and quantitatively resemble Saturn's Chandra spectrum very
well.
Key words: planets and satellites: general -- planets and satellites individual: Saturn -- X-rays: general
Offprint request: J.-U. Ness, jness@hs.uni-hamburg.de
© ESO 2004
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