A fast X-ray timing capability on XEUS

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dc.creatorBarret, D.
dc.creatorSkinner, G.
dc.creatorKendziorra, E.
dc.creatorStaubert, R.
dc.creatorStella, L.
dc.creatorVan der Klis, M.
dc.date2002-02-25
dc.date.accessioned2026-07-07T02:02:54Z
dc.date.available2026-07-07T02:02:54Z
dc.descriptionThe Rossi X-ray Timing Explorer has demonstrated that fast X-ray timing can be used to probe strong gravity fields around collapsed objects and constrain the equation of state of dense matter in neutron stars. These studies require extremely good photon statistics. In view of the huge collecting area of its mirrors, XEUS could make a unique contribution to this field. For this reason, it has been proposed to include a fast X-ray timing capability in the focal plane of the XEUS mirrors. We outline the scientific motivation for such a capability, present some sensitivity estimates, and discuss briefly a possible detector implementation.
dc.description4 pages, 3 figures + latex document class file. Proc. Symposium "New Visions of the X-ray Universe in the XMM-Newton and Chandra Era", 26-30. November 2001, ESTEC, The Netherlands
dc.identifierhttps://arxiv.org/abs/astro-ph/0202451
dc.identifierhttp://arxiv.org/abs/astro-ph/0202451
dc.identifierESA SP-488, August 2002, ed. F. Jansen
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/4206
dc.subjectAstrophysics
dc.titleA fast X-ray timing capability on XEUS
dc.typetext

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