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dc.contributor.authorJohnson, T.J.
dc.contributor.authorVenter, C.
dc.contributor.authorHarding, A.K.
dc.contributor.authorGuillemot, L.
dc.contributor.authorFermi LAT
dc.date.accessioned2019-04-04T13:04:22Z
dc.date.available2019-04-04T13:04:22Z
dc.date.issued2011
dc.identifier.citationJohnson, T.J. et al. 2011. Observations and modeling of gamma-ray millisecond pulsars seen with the Fermi LAT. AIPC, 1357:237-240. [https://arxiv.org/pdf/1012.3635.pdf]en_US
dc.identifier.urihttp://hdl.handle.net/10394/32149
dc.identifier.urihttps://arxiv.org/pdf/1012.3635.pdf
dc.description.abstractWe 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 modeldependent confidence contours for the viewing geometry in these systems which are complementary to those from polarization measurementsen_US
dc.language.isoenen_US
dc.publisherAIPCen_US
dc.subjectGamma rays: observationsen_US
dc.subjectPulsars: milliseconden_US
dc.titleObservations and modeling of gamma-ray millisecond pulsars seen with the Fermi LATen_US
dc.typePresentationen_US
dc.contributor.researchID12006653 - Venter, Christo


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