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2018

Sandoval, L. E. Rivera, Maccarone, T. J., Corsi, A. et al.

Supernova (SN) 2018cow (or AT2018cow) is an optical transient detected in the galaxy CGCG 137-068.

It has been classified as a SN due to various characteristics in its optical spectra.
The transient is also a bright X-ray source.
We present results of the analysis of ~62ks of X-ray observations taken with the Neil Gehrels Swift Observatory over 27 days.

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