Observations and modeling of gamma-ray millisecond pulsars seen with the Fermi LAT
| dc.contributor.author | Johnson, T.J. | |
| dc.contributor.author | Venter, C. | |
| dc.contributor.author | Harding, A.K. | |
| dc.contributor.author | Guillemot, L. | |
| dc.contributor.author | Fermi LAT | |
| dc.contributor.researchID | 12006653 - Venter, Christo | |
| dc.date.accessioned | 2019-04-04T13:04:22Z | |
| dc.date.available | 2019-04-04T13:04:22Z | |
| dc.date.issued | 2011 | |
| dc.description.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 modeldependent confidence contours for the viewing geometry in these systems which are complementary to those from polarization measurements | en_US |
| dc.identifier.citation | Johnson, 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.uri | http://hdl.handle.net/10394/32149 | |
| dc.identifier.uri | https://arxiv.org/pdf/1012.3635.pdf | |
| dc.language.iso | en | en_US |
| dc.publisher | AIPC | en_US |
| dc.subject | Gamma rays: observations | en_US |
| dc.subject | Pulsars: millisecond | en_US |
| dc.title | Observations and modeling of gamma-ray millisecond pulsars seen with the Fermi LAT | en_US |
| dc.type | Presentation | en_US |