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NASA NTRS · 19930039411

The X-ray Timing Explorer

Abstract

The capabilities of the X-ray Timing Explorer (XTE) are described with particular attention paid to current scientific problems it will address from galactic neutron star systems to active galactic nuclei. It features a low-background continuous 2-200 keV response with large apertures (a 0.63 sq m proportional counter array and a 0.16 sq m dual rocking NaI/CsI scintillation array). Rapid response (in hours) to temporal phenomena, e.g. transients, is obtained by virtue of a scanning all-sky monitor and rapid maneuverability. XTE will carry out detailed energy-resolved studies of phenomena close to neutron stars (e.g. QPO's) because of its submillisecond timing, its high telemetry rates, and the high throughput of its data system.

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BibTeXRIS

Bradt, H. V., Levine, A. M., Morgan, E. H., Remillard, R. A., Swank, J. H., Dingus, B. L., Holt, S. S., Jahoda, K. M., Rotschild, R. E., Gruber, D. E.. 1990-01-01. The X-ray Timing Explorer. https://ntrs.nasa.gov/citations/19930039411

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