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A three bright X-ray non-target sources are detected in the field of theseyfert 1 galaxy MKN 205. These sources are classified as optically Early-typegalaxy, BLAGN, and NELG (NED, SIMBAD, and AXIS). The spectrum analysis is madefor these objects using thermal models and non-thermal models, modified byinterstellar absorption. In some objects we can not distinguish between thethermal and non-thermal models of the hard components from the spectrum alone.The presence of intrinsic absorption is tested by photoelectric absorption atthe redshift of the sources, and we assumed the flux distribution is affectedby the intrinsic absorption in some sources. A black body component used totest the presence of soft excess in some spectra, which has been interpreted asprimary emission from the accretion disc or as secondary radiation form thereprocessing of the hard X-ray in the surface layers of the disc.

X-ray Bright Sources in the Field of Active Galactic Nuclei MKN 205