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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, 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.
SECTIONS
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Participants
Paul Ray <paul.ray@nrl.navy.mil >,
Damien Parent <damien.parent.ctr.fr@nrl.navy.mil >,
Matthew Kerr,
Pablo Saz Parkinson,
Michael Dormody, and others...
Timing solutions
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label | 24 months |
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Updated : January 2011
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List of Pulsars timing by the LAT
Pulsar Name | Comments | PAR | Residuals | RMS (ms) |
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J0007+7303 | in CTA1 | 2.9 | ||
J0205+6449 | in 3C 58 |
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J0357+3206 |
| 6.4 | ||
J0633+0632 | ||||
J0633+1746 | RESIDS Geminga | 1.7 | ||
J1826-1256 |
| 0.6 | ||
J2021+3651 |
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J2229+6114 | in Boomerang |
| 0.5
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Timing solutions
Composition Setup |
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- Validity range of the timing models : 24 months from 2008 August 4
- Timing models are available here:
Code Block http://www.slac.stanford.edu/~parent/LATPulsarTimingModels/24months/