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You are free to use these LAT timing solutions to fold your data. If you publish work based on these models, please reference Ray, Kerr, Parent et al. (2011) and this page in your publication. The primary intent is to support pulsar analyses requiring timing ephemerides, such at phase-resolved spectroscopy and analyses of sources close to bright pulsars through the use of pulsar `gating'. If, on the other hand, you want to publish something based on the values of the timing model parameters (e.g. timing positions, glitch parameters, etc...) we ask that you contact us first because there may be important caveats or publication plans.
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Participants
Paul Ray, Damien Parent, Matthew Kerr, Pablo Saz Parkinson, Michael Dormody, and others...
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