IN PREPARATION
Overview
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 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.
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These timing solutions are valid from 2008 August 4 to 2010 August.