In this research, we study the energy, flux values of Sagittarius A* black hole from various telescopes like Chandra Shekhar X-Ray, FERMI. It is found that from recent data from a similarly scattered screen is actually not directly in the galactic center. It is also found that variability appears to get stronger with frequency. This is compatible with plasma blobs streaming outward (in a jet or otherwise) and expanding adiabatically. The comparison of flux values and energy measured by different observatories are also observed and discussed.
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Lamichhane et al. (2024) studied this question.
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