LAT Gamma-ray Pulsar Timing Models

• Overview
• Participants
• List of pulsars
• LAT timing solutions

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. (2011, ApJS, accepted 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 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.

Participants

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

Timing solutions

The timing solutions will be updated every 3-6 months.

Comments

• The LAT solutions can be used with the Fermi plugin available in the TEMPO2 distribution.

List of Pulsars timed by the LAT