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Study of Intra-Day Flux Distributions of Blazars Using XMM-Newton Satellite
We present a study of the flux distribution of a sample of 15 Intermediate and Low-energy peaked blazars using XMM-Newton observations in a total of 57 epochs on short-term timescales. We characterise the X-ray variability of all of the light curves using excess fractional variability amplitude and found that only 24 light curves in 7 sources are significantly variable. In order to characterise the origin of X-ray variability in these blazars, we fit the flux distributions of all these lightdoi:10.3390/universe8110578 fatcat:tzpgabuzgrhg5bujsvkhbbdmka