Author(s): A. Abdo A., Ajello M., Antolini E., Baldini L., Ballet J., Barbiellini G., G. Baring M., Bastieri D., Bechtol K., Bellazzini R., Berenji B., Bruel P., Cohen-Tanugi J., Dumora D., Fortin P., A. Grenier I., Grondin M.-H., Guillemot L., Guiriec Sylvain, Knodlseder J., Lemoine-Goumard M., Lott B., Nuss E., Parent D., Pelassa V., Piron F., Reposeur T., Sgro C., A. Smith D., Tibaldo L.
(Article) Published:
The Astrophysical Journal / The Astrophysical Journal Letters, vol. 720 p.26-40 (2010)
Links openAccess full text : 
Ref HAL: in2p3-00530021_v1
Ref Arxiv: 1008.0008
DOI: 10.1088/0004-637X/720/1/26
Ref. & Cit.: NASA ADS
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Abstract:
The Fermi Large Area Telescope (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 from the analysis of 13 months of LAT data for three of these pulsars (PSR J1057-5226, PSR J1709-4429, and PSR J1952+3252) each of which had some unique feature among the EGRET pulsars. The excellent sensitivity of LAT allows more detailed analysis of the evolution of the pulse profile with energy and also of the variation of the spectral shape with phase. We measure the cutoff energy of the pulsed emission from these pulsars for the first time and provide a more complete picture of the emission mechanism. The results confirm some, but not all, of the features seen in the EGRET data.
Comments: Accepted for publication in ApJ. 45 pages, 12 figures, 11 tables. Corresponding authors: O. Celik, F. Gargano, T. Reposeur, D.J. Thompson