Abdo, A. A.A. A.AbdoAckermann, M.M.AckermannAjello, M.M.AjelloTosti, G.G.TostiGasparrini, DarioDarioGasparrini2020-09-172020-09-172010-04-01https://hdl.handle.net/20.500.13025/1762The Astrophysical Journal, Volume 712, Issue 2, pp. 1209-1218 (2010).The discovery of the gamma-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 10<SUP>34</SUP> erg s<SUP>-1</SUP>, and a large off-peak (OP) emission component, making it quite unusual among the known gamma-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.gamma rays generalpulsars generalpulsars individual PSR J1836+592510.1088/0004-637X/712/2/1209http://adsabs.harvard.edu/abs/2010ApJ...712.1209A2010ApJ...712.1209A