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Por favor, use este identificador para citar o enlazar a este item: http://hdl.handle.net/10261/239688
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dc.contributor.authorBrand, T.es_ES
dc.contributor.authorWilms, Jörnes_ES
dc.contributor.authorDauser, T.es_ES
dc.contributor.authorPeille, Philippees_ES
dc.contributor.authorCobo, Beatrizes_ES
dc.contributor.authorCeballos, María Teresaes_ES
dc.contributor.authorHartog, Roland H. denes_ES
dc.contributor.authorKaastra, Jellees_ES
dc.contributor.authorO'Brien, P.es_ES
dc.contributor.authorBarcons, Xavieres_ES
dc.contributor.authorPiro, Luigies_ES
dc.contributor.authorHerder, J. W. denes_ES
dc.contributor.authorBarret, Didieres_ES
dc.date.accessioned2021-04-30T11:51:07Z-
dc.date.available2021-04-30T11:51:07Z-
dc.date.issued2016-
dc.identifier.citationProceedings of SPIE 9905: 99055F (2016)es_ES
dc.identifier.urihttp://hdl.handle.net/10261/239688-
dc.descriptionEvent: SPIE Astronomical Telescopes + Instrumentation, 2016, Edinburgh, United Kingdom.es_ES
dc.description.abstractWe present simulations of the detection probability for absorption lines from ions in the warm and hot ionized medium (WHIM) with Athena in the spectra of Gamma-ray burst afterglows. The simulations are based on Swift XRT lightcurves of these afterglows and are performed using the end-to-end simulation framework SIXTE. We simulate both the case of single and multiple absorption lines, as well as results for line searches in absorption structures from a more complex medium. We show that the Athena X-IFU can detect WHIM lines with strong Ovii lines (equivalent widths larger than 0.14 eV) in spectra containing 3 x 106 counts.es_ES
dc.description.sponsorshipThis work made use of data supplied by the UK Swift Science Data Centre at the University of Leicester and of ISIS functions (ISISscripts) provided by ECAP/Remeis observatory and MIT (http://www.sternwarte. uni-erlangen.de/isis/). We thank J.E. Davis for the development of the SLXfig module, which was used to create all gures in this paper. We acknowledge funding by the Deutsches Zentrum f ur Luft- und Raumfahrt contract 50QR1402.es_ES
dc.language.isoenges_ES
dc.publisherSPIE digital libraryes_ES
dc.relation.isversionofPublisher's versiones_ES
dc.rightsopenAccesses_ES
dc.titleObserving the WHIM with Athenaes_ES
dc.typecomunicación de congresoes_ES
dc.identifier.doi10.1117/12.2234442-
dc.description.peerreviewedPeer reviewedes_ES
dc.relation.publisherversionhttps://doi.org/10.1117/12.2234442es_ES
dc.identifier.e-issn1996-756X-
dc.contributor.funderUniversity of Leicesteres_ES
dc.relation.csicSíes_ES
oprm.item.hasRevisionno ko 0 false*
dc.identifier.funderhttp://dx.doi.org/10.13039/501100000738es_ES
dc.type.coarhttp://purl.org/coar/resource_type/c_5794es_ES
item.openairetypecomunicación de congreso-
item.languageiso639-1en-
item.grantfulltextopen-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextWith Fulltext-
item.cerifentitytypePublications-
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