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Analysis reveals XID 912 as an off-nuclear ultraluminous x-ray source, suggesting unique properties in celestial observations.
In the 7 Ms Chandra Deep Field-South catalog, only one source, XID 912, was highly significantly detected in X-rays but had no formally reported counterparts in the UV, optical, infrared, or radio bands. We identified its potential JWST and Very Large Telescope VIMOS counterparts and measured the corresponding aperture photometry to construct its spectral energy distribution (SED). We fitted this SED using CIGALE . The results indicate that the source is most likely an off-nuclear ultraluminous X-ray source, rather than a background active galactic nucleus.
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Sullivan et al. (2025) studied this question.
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