About: Detection of Saturnian X-ray emission with XMM-Newton

Documentation

scienceplus.abes.fr version Bêta

scienceplus.abes.fr | explorer

À propos de : Detection of Saturnian X-ray emission with XMM-Newton Goto Sponge NotDistinct Permalink

Attributs	Valeurs
type	work Article
Is Part Of	http://hub.abes.fr/edp/periodical/aa/2004/volume_414/issue_3/w
Subject	X-rays: general Letters Letter to the editor planets and satellites: general planets and satellites individual: Saturn
Title	Detection of Saturnian X-ray emission with XMM-Newton
Date	2004-01-01(xsd:dateTime)
has manifestation of work	http://hub.abes.fr/edp/periodical/aa/2004/volume_414/issue_3/aafl052/m/print http://hub.abes.fr/edp/periodical/aa/2004/volume_414/issue_3/aafl052/m/web
related by	http://hub.abes.fr/edp/periodical/aa/2004/volume_414/issue_3/aafl052/authorship/1 http://hub.abes.fr/edp/periodical/aa/2004/volume_414/issue_3/aafl052/authorship/3 http://hub.abes.fr/edp/periodical/aa/2004/volume_414/issue_3/aafl052/authorship/2
Author	Ness, J.-U. Robrade, J. Schmitt, J. H. M. M.
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.
article type	letter
publisher identifier	aafl052
Date Copyrighted	2004-01-01(xsd:dateTime)
Rights	© ESO, 2004
Rights Holder	ESO
is part of this journal	Astronomy & Astrophysics
is primary topic of	http://hub.abes.fr/edp/periodical/aa/2004/volume_414/issue_3/aafl052/w/record

Alternative Linked Data Documents: ODE Content Formats:

RDF

ODATA

Microdata