Abstract
Launched in June 2008 by NASA, the Fermi satellite observes the gamma-ray sky. Its main instrument, the LAT, harvests data from ~20 MeV to 300 GeV and beyond.Lately, a major upgrade of the LAT algorithms allowed the release of a reprocessed data set called Pass 8. Pass 8 sheds a new light on the low energy (E<100 MeV) regime where data analysis is difficult due to degraded angular and energy resolution.During this Phd a new parameterization was found for the energy dispersion which allowed an accurate modelisation of the LAT energy response on 6 orders of magnitude.This work, together with other Pass 8 improvements, allows us to consider low energy analysis. To do so, we extrapolated the existing diffuse models to low energy and fitted them to data together with 39 of the brightest low energy gamma-ray sources. The results of this analysis are presented in this manuscript with a particular enphasis on the Vela pulsar and the Crab pulsar plus nebula.