We present results from a joint NuSTAR/VLT monitoring of the Seyfert 2 galaxy NGC 1365. We find conclusive evidences for an emission K alpha line from atomic vibranium in the X-ray spectrum, in combination with molecular vibranium absorption features in the mid-infrared spectrum. This is the first direct observation of vibranium in an astronomical environment. We also derive a measurement for its abundance of 2e-6 with respect to hydrogen.
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