Astronomy and Astrophysics – Astrophysics – High Energy Astrophysical Phenomena
Scientific paper
2010-11-23
Proceedings of High Time Resolution Astrophysics IV - The Era of Extremely Large Telescopes, PoS(HTRA-IV)050, 2010
Astronomy and Astrophysics
Astrophysics
High Energy Astrophysical Phenomena
5 pages, 2 figures, to be published in the proceedings of High Time Resolution Astrophysics IV - The Era of Extremely Large Te
Scientific paper
Usually, positions of spacecraft on interplanetary or deep space missions are determined by radar tracking from ground stations, a method by which uncertainty increases with distance from Earth. As an alternative, a spacecraft equipped with e.g. an X-ray telescope could determine its position autonomoulsy via onboard analysis of X-ray pulsar signals. In order to find out which pulsars are best suited for this approach and what accuracy can be achieved, we build up a database containing the temporal emission characteristics of the ~ 60 X-ray pulsars for which a pulsed radiation has been detected by mid 2010.
Becker Werner
Bernhardt Mike Georg
Prinz Tobias
Walter Ulrich
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