| dc.contributor.author | Johnson, T.J. | |
| dc.contributor.author | Venter, C. | |
| dc.contributor.author | Harding, A.K. | |
| dc.contributor.author | Grove, J.E. | |
| dc.date.accessioned | 2019-04-04T08:09:02Z | |
| dc.date.available | 2019-04-04T08:09:02Z | |
| dc.date.issued | 2012 | |
| dc.identifier.citation | Johnson, T.J. et al. 2012. Modeling the pulse profiles of millisecond pulsars in the second LAT catalog of γ-ray pulsars. 5th International Meeting on High Energy Gamma-Ray Astronomy, 9-13 July, Heidelberg, Germany. AIP conference series, 1505: 325-328. [https://doi.org/10.1063/1.4772263] | en_US |
| dc.identifier.isbn | 978-0-7354-1123-4 | |
| dc.identifier.uri | http://hdl.handle.net/10394/32139 | |
| dc.identifier.uri | https://aip.scitation.org/doi/pdf/10.1063/1.4772263?class=pdf | |
| dc.identifier.uri | https://doi.org/10.1063/1.4772263 | |
| dc.description.abstract | Significant γ-ray pulsations have been detected from ∼40 millisecond pulsars (MSPs) using 3 years of sky-survey data from the Fermi LAT and radio timing solutions from across the globe. We have fit the radio and γ-ray pulse profiles of these MSPs using geometric versions of slot gap and outer gap γ-ray emission models and radio cone and core models. For MSPs with radio and γ-ray peaks aligned in phase we also explore low-altitude slot gap γ-ray models and caustic radio models. The best-fit parameters provide constraints on the viewing geometries and emission sites. While the exact pulsar magnetospheric geometry is unknown, we can use the increased number of known γ-ray MSPs to look for significant trends in the population which average over these uncertainties | en_US |
| dc.language.iso | en | en_US |
| dc.publisher | AIP | en_US |
| dc.title | Modeling the pulse profiles of millisecond pulsars in the second LAT catalog of γ-ray pulsars | en_US |
| dc.type | Presentation | en_US |
| dc.contributor.researchID | 12006653 - Venter, Christo | |
