High-energy Observations Of Pulsars J1057-5226, J1709-4429 And J1952+3252 With The Fermi Large Area Telescope

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The Fermi-LAT data have confirmed the pulsed emission from all six high-confidence gamma-ray pulsars previously known from the EGRET observations. We report results obtained with the analysis of 9 months of LAT data for three of these pulsars: J1057-5226, J1709-4429, and J1952+3252.
Each of these pulsars had some unique feature among the EGRET pulsars. With the excellent sensitivity of LAT, it was possible to perform a more sensitive light curve and spectral analysis of these pulsars to investigate these features with higher statistics. Moreover, the broader energy range of the LAT allowed us to measure the cutoff energy of pulsed emission from these pulsars for the first time and provided a more complete picture of the emission mechanism. The results confirm some, but not all, of the features of the EGRET results.

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