Abstract
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 built 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.
| Original language | English |
|---|---|
| Journal | Proceedings of Science |
| Volume | 108 |
| State | Published - 2010 |
| Event | 4th High Time Resolution Astrophysics - The Era of Extremely Large Telescopes, HTRA 2010 - Crete, Greece Duration: 5 May 2010 → 7 May 2010 |
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