LAT Gamma-ray Pulsar Timing Models

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

• Overview
• Participants
• List of pulsars
• LAT solutions

Participants

Paul Ray, Damien Parent, Matthew Kerr, Pablo Saz Parkinson, Michael Dormody, and others...

List of Pulsars timing by the LAT

Timing solutions

• Validity range of the timing models : 24 months from 2008 August 4

• Timing models are available here:

  http://www.slac.stanford.edu/~parent/LATPulsarTimingModels/24months/