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dc.contributor.authorAbdo, A.A.en_US
dc.contributor.authorVenter, C.en_US
dc.contributor.authorAckermann, M.en_US
dc.contributor.authorAjello, M.
dc.contributor.authorAtwood, W.B.
dc.date.accessioned2012-02-29T09:51:53Z
dc.date.available2012-02-29T09:51:53Z
dc.date.issued2010en_US
dc.identifier.citationAbdo, A.A. et al. 2010. Fermi large area telescope observations of PSR J1836+5925. Astrophysical journal, 712:1209-1218. [https://doi.org/10.1088/0004-637X/712/2/1209]en_US
dc.identifier.issn0004-637Xen_US
dc.identifier.issn1538-4357 (Online)en_US
dc.identifier.urihttp://hdl.handle.net/10394/6069
dc.identifier.urihttps://doi.org/10.1088/0004-637X/712/2/1209
dc.description.abstractThe discovery of the γ-ray pulsar PSR J1836+5925, powering the formerly unidentified EGRET source 3EG J1835+5918, was one of the early accomplishments of the Fermi Large Area Telescope (LAT). Sitting 25° off the Galactic plane, PSR J1836+5925 is a 173 ms pulsar with a characteristic age of 1.8 million years, a spindown luminosity of 1.1 × 1034 erg s–1, and a large off-peak (OP) emission component, making it quite unusual among the known γ-ray pulsar population. We present an analysis of one year of LAT data, including an updated timing solution, detailed spectral results, and a long-term light curve showing no indication of variability. No evidence for a surrounding pulsar wind nebula is seen and the spectral characteristics of the OP emission indicate it is likely magnetospheric. Analysis of recent XMM-Newton observations of the X-ray counterpart yields a detailed characterization of its spectrum, which, like Geminga, is consistent with that of a neutron star showing evidence for both magnetospheric and thermal emission
dc.publisherIOP Publishingen_US
dc.titleFermi large area telescope observations of PSR J1836+5925en_US
dc.contributor.researchID12006653 - Venter, Christo


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