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This page is for distribution of pulsar timing models made by the LAT team directly from LAT gamma-ray data, independent of any radio timing data that may exist. We use the methods documented in Ray, Kerr, Parent et al. (20102011, ApJApJS, submittedaccepted arXiv:1011.2468 ). The primary focus is on the blind search pulsars and other pulsars that are not easily timed in the radio or X-ray bands. If you would like a particular pulsar added to this page, please contact us. This work is being supported by the Fermi Cycle 3 Guest Observer program.
You are free to use the these LAT timing solutions to fold your data. Any references toIf you publish work based on these models, please reference Ray, Kerr, Parent et al. (2011) and this page in either your publication or the acknowledgements will be appreciate.
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