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tokens: ACKNOWLEDGEMENTS This research has made use of data obtained from the High Energy Astrophysics Science Archive Research Center (HEASARC), provided by NASA’s Goddard Space Flight Center. This research has made use of the NuSTAR Data Analysis Software ( nustardas ) jointly developed by the ASI Science Data Center (ASDC, Italy) and the California Institute of Technology (USA). RS and AJ acknowledge the financial support from the University Grants Commission (UGC), India, under the SRF and MANF-SRF schemes, respectively.