...
Model | RA(°) | DEC(°) | Semi Major Axis (°) | Semi Minor Axis (°) | Pos.Ang.(°) |
283,990 | 1,355 | 0,300 | 0,190 | 327,000 | |
Pass 6 | 284.015(+/-0.004) | 1.392(+/-0.005) | 0.335(+0.117 -0.086) | 0.207 (+0.023 -0.021) | 330+/- 25 |
Pass 7 | 284.000(+/-0.006) | 1.374(+/-0.006) | 0.332(+0.109/-0.079) | 0.205 (+0.021/-0.017) | 327 +/-22 |
...
The second part summarize the data I used.
The third part (Fermi data analysis) is divided in 2
- Search for pulsation. -> No pulsed emission
- Spatial and spectral analysis
- Spatial
- Spectral
The discussion begins with the SED modeling and present the gamma-ray luminosity and efficiency.
I would like to show 3 figures which are th Fig. 4, 8 and 11.
The draft is coming soon.
Bibliography :
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(3) Aharonian et al., A&A, 477, 353-363, 2008
(4) Cordes, J. M., & Lazio, T. J. W. 2002, preprint (astro-ph/0207156)
(5) Vincent, M., Thesis : “Nebuleuse de pulsars : sondage profond de la Galaxie au TeV et études multi-longueur d'onde”.
(6) Sugizaki et al., ApJ Supplement Series, 134, 77-102, 2001
(7) Ackermann et al., ApJ, 726, 35-102, 2011