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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. (2010, ApJ, submitted 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 LAT timing solutions to fold your data, however, we ask that you please refer to Ray, Kerr, Parent et al. in either your publication or the acknowledgements.
Participants
Paul Ray, Damien Parent, Matthew Kerr, Pablo Saz Parkinson, Michael Dormody, and others...
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Timing solutions
The timing solutions will be updated every 3-6 months.
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| - Validity range of the timing models : 24 months from 2008 August 4
- LAT Timing models are available HERE.
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- The LAT solutions can be used with the TEMPO2 '' Fermi '' plugin.PSR xxx cannot be timed over the whole LAT missionplugin available in the TEMPO2 distribution.
List of Pulsars timing by the LAT
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