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arXiv · 1012.3922

Pulsar Timing with the Fermi LAT

Paul S. Ray·Matthew Kerr·Damien Parent·the Fermi PSC
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Abstract

We present an overview of precise pulsar timing using data from the Large Area Telescope (LAT) on Fermi. We describe the analysis techniques including a maximum likelihood method for determining pulse times of arrival from unbinned photon data. In addition to determining the spindown behavior of the pulsars and detecting glitches and timing noise, such timing analyses allow the precise determination of the pulsar position, thus enabling detailed multiwavelength follow up.

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Paul S. Ray, Matthew Kerr, Damien Parent, the Fermi PSC. 2010-12-17. Pulsar Timing with the Fermi LAT. https://doi.org/10.1063/1.3615094

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