| Name: | Hritwik Bora |
| Affiliation: | Tezpur University |
| Conference ID : | ASI2024_832 |
| Title : | Jet power of Mkn 501 from Broadband SED modeling |
| Authors : | Hritwik Bora, Rukaiya Khatoon, Ranjeev Misra, Rupjyoti Gogoi |
| Authors Affiliation: | 1 Hritwik Bora, Rupjyoti Gogoi, Department of Physics, Tezpur University,Tezpur - 784028, Assam, India
2 Rukaiya Khatoon, Centre for Space Research, North-West University, South Africa
3 Ranjeev Misra, Inter-University Centre for Astronomy and Astrophysics, Post Bag 4, Ganeshkhind, Pune, Maharashtra - 411007 |
| Mode of Presentation: | Poster |
| Abstract Category : | High Energy Phenomena, Fundamental Physics and Astronomy |
| Abstract : | We performed the X-ray, Ultraviolet (UV), and Gamma-ray analysis of high energy peaked (HBL) blazar source Mkn 501 using Swift-XRT/UVOT, NuSTAR, Fermi-LAT observations. The simultaneous Swift-XRT/UVOT and NuSTAR observations between 2013 and 2022 are taken in this study with 4 months of Fermi-LAT observations against each NuSTAR observation. We carried out the Broadband SED modeling considering the underlying process to be Synchrotron and Synchrotron Self Compton (SSC) emission. Also, we fitted the spectrum with empirical models like the Log-parabola and Broken Power Law along with physical models like power-law particle distribution with maximum electron energy, and energy-dependent acceleration and diffusion models. For all the particle distributions we obtained the jet powers and further checked for the variation of the jet power for different bulk lorentz factors. We briefly discuss the obtained findings. |
