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We present a summary of gamma-ray millisecond pulsar (MSP) observations withthe Fermi Large Area Telescope. The radio and gamma-ray light curves of theseMSPs have been modeled in the framework of the retarded vacuum dipole magneticfield. Likelihood fitting of the radio and gamma-ray light curves withgeometric emission models allows us to give model-dependent confidence contoursfor the viewing geometry in these systems which are complementary to those frompolarization measurements.

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