Long term study of the light curve of PKS 1510-089 in GeV energies
arXiv:1706.02133 · doi:10.3847/1538-4357/aa78f4
Abstract
We have analyzed data from the Flat Spectrum Radio Quasar PKS 1510-089 collected over a period of 8 years from August 2008 to December 2016 with the Fermi-LAT. We have identified several flares of this highly variable source, studied their temporal and spectral properties in detail and compared with previous works on flares of PKS 1510-089. Five major flares and few sub-flares/sub-structures have been identified in our study. The fastest variability time is found to be 1.300.18 hr between MJD 55852.063 and 55852.188 where we estimate the minimum size of the emission region to be cm. In most of the flares the spectral energy distributions are better fitted with Logparabolic distribution compared to simple Power law or Power law with exponential cut-offs. This has strong physics implications regarding the nature of the high energy gamma-ray emission region.
arXiv comment29 pages, 29 figures, Accepted in ApJ
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- Detection of persistent VHE gamma-ray emission from PKS 1510-089 by the MAGIC telescopes during low states between 2012 and 2017
- Fermi-Large Area Telescope observations of the brightest Gamma-ray flare ever detected from CTA 102
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- Exploring the origin of multiwavelength activities of high-redshift FSRQ PKS 1502+106 during 2014-2018
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