Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/7967
Title: Multiwavelength temporal and spectral analysis of Blazar S5 1803+78
Authors: Priya, Shruti
Prince, Raj
Agarwal, Aditi
Bose, Debanjan
Ozdonmez, Aykut
Ege, Ergun
Keywords: Galaxies: Active
X-rays Galaxies
Gamma-rays Galaxies
galaxies: Jets
BL Lacertae objects
Issue Date: Jun-2022
Publisher: Oxford University Press on behalf of the Royal Astronomical Society
Citation: Monthly Notices of Royal Astronomical Society, 2022, Vol. 513, p2239
Abstract: Blazars are a class of AGN, one of their jets is pointed towards the earth. Here, we report about the multiwavelength study for blazar S5 1803+78 between MJD 58727 and MJD 59419. We analysed gamma-ray data collected by Fermi-LAT, X-ray data collected by Swift-XRT & NuSTAR, and optical photons detected by Swift-UVOT & TUBITAK observatory in Turkey. Three flaring states are identified by analysing the gamma-ray light curve. A day-scale variability is observed throughout the flares with the similar rise and decay times suggesting a compact emission region located close to the central engine. Cross-correlation studies are carried out between gamma-ray, radio, and X-ray bands, and no significant correlation is detected. The gamma-ray and optical emission are significantly correlated with zero time lag suggesting a co-spatial origin of them. The broad-band spectral energy distribution (SED) modelling was performed for all the flaring episodes as well as for one quiescent state for comparison. SEDs are best fitted with the synchrotron-self Compton (SSC) model under a one-zone leptonic scenario. The SED modelling shows that to explain the high flaring state, strong Doppler boosting is required.
Description: Restricted Access. An open-access version is available at arXiv.org (one of the alternative locations)
URI: http://hdl.handle.net/2289/7967
ISSN: 0035-8711
1365-2966 (Online)
Alternative Location: https://ui.adsabs.harvard.edu/abs/2022MNRAS.513.2239P/abstract
https://arxiv.org/abs/2204.04739
https://doi.org/10.1093/mnras/stac1009
Copyright: 2022 The Author(s)
Appears in Collections:Research Papers (A&A)

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