Measuring Gravitational Acceleration Using X-Ray Pulsars for Deep Space Navigation Algorithm Initialization
A method for measuring gravitational acceleration using x-ray pulsars is presented. Using a Maximum Likelihood Estimator, x-ray photon arrival times are processed to generate position, velocity and acceleration measurements. This method is validated in simulation. To determine how well this estimator can perform, a Cramer-Rao lower bound analysis is presented.
Authors
- Demoz Gebre-Egziabher (ORCID: https://orcid.org/0000-0001-6874-2594)
- K. Houser
Publication Details
- Journal
- Proceedings of the Satellite Division's International Technical Meeting (Online)/Proceedings of the Satellite Division's International Technical Meeting (CD-ROM)
- Published
- 2024-10-09
- DOI
- https://doi.org/10.33012/2024.19925
- Primary Topic
- Pulsars and Gravitational Waves Research
- Type
- article
- Field-Weighted Citation Impact
- 0.00