Observations and Modeling of Gamma-ray Millisecond Pulsars seen with the Fermi LAT

Tyrel J. Johnson; Christo Venter; Alice K. Harding; Lucas Guillemot

doi:10.1063/1.3615124

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arXiv · 1012.3635

Observations and Modeling of Gamma-ray Millisecond Pulsars seen with the Fermi LAT

Tyrel J. Johnson·Christo Venter·Alice K. Harding·Lucas Guillemot

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Abstract

We present a summary of gamma-ray millisecond pulsar (MSP) observations with the Fermi Large Area Telescope. The radio and gamma-ray light curves of these MSPs have been modeled in the framework of the retarded vacuum dipole magnetic field. Likelihood fitting of the radio and gamma-ray light curves with geometric emission models allows us to give model-dependent confidence contours for the viewing geometry in these systems which are complementary to those from polarization measurements.

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Tyrel J. Johnson, Christo Venter, Alice K. Harding, Lucas Guillemot. 2010-12-16. Observations and Modeling of Gamma-ray Millisecond Pulsars seen with the Fermi LAT. https://doi.org/10.1063/1.3615124

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